This paper presents an exploration of solar flares and solar radio bursts(SRBs) associated with β-γ-δ class active regions (ARs) during the ascending phase of solar cycle 25th, spanning from January 2022 to May 2024. The β-γ-δ ARs have complex magnetic fields with bipolar configurations, which are conducive to the production of intense solar flares. During solar flares, powerful electromagnetic (EM) radiation including solar radio bursts (SRBs) penetrates the outside of the Sun. The investigation was started by collecting the number of β-γ-δ, solar flares and SRBs for statistical evaluation. The details of AR such as the date and number of the active region of β-γ-δ were obtained from the Space Weather Live website. Then, the associated number of solar flares in all classes (Class-B, Class-C, Class-M and Class-X) from SWPC, NOAA and SRBs of Type II, Type III and Type IV from the CALLISTO spectrometer were calculated and recorded. In order to observe changes over the years, the data for solar flares and SRBs were analyzed separately for 2022, 2023, and 2024 and plotted in histograms. The results show that the average occurrence of β-γ-δ ARs in 2024 was 6 days and it was higher than compared to in 2023 and 2022 which had averages of 2 and 3 days, respectively. The production of Class-C, Class-M, and Class-X flares demonstrated significant trends with the ascending phase of the solar cycle. The highest number of Class-X flares occurred in AR 13664, with 10 flares recorded over 9 days. Moreover, the number of SRBs included 12 Type II bursts and 6 Type IV bursts, with the majority of days having both types of bursts. Additional factors contributing to the production number of solar flares and SRBs from β-γ-δ ARs have been studied and discussed in this paper.