The galaxy presents a roughly circular morphology. A bright, centrally concentrated region is evident, suggesting the presence of a significant bulge or active galactic nucleus. The central region exhibits a bluish hue, indicating the presence of younger, hotter stars and ongoing star formation. Fainter, less defined spiral arms emanate from the central region. These arms are somewhat clumpy and asymmetrical, with regions of increased brightness possibly indicating HII regions or star forming areas. There may be minor tidal disturbance or a close companion, as there is some asymmetry in the outer edges of the disc, hinting at gravitational interaction. Overall, the galaxy seems to be actively forming stars.
