The galaxy presents as a roughly elliptical structure with a dominant, centrally concentrated bulge. The color gradient indicates a relatively older stellar population in the core, trending towards redder wavelengths. Fainter, bluer regions extend outwards from the central bulge, hinting at the presence of a younger stellar population. There appears to be a slight disk feature. The disk component shows a more active star formation region and younger star clusters. The outer edges of the disk fade, suggesting a gradual decrease in stellar density. There is some distortion, which could be attributed to a possible minor interaction or disturbance.
