The galaxy presents as a somewhat elliptical, though nearly lenticular, structure. A prominent central bulge exhibits a yellowish-white hue, indicating a population of older stars. Fainter and bluer light extends from the central region, suggesting the presence of a relatively flat disk. The disk component shows some texture and irregularity, hinting at possible arm-like structures or minor disturbances in the galaxy's morphology, but these features are not strongly defined. Overall, the galaxy appears relatively smooth, with no clear signs of major mergers or significant tidal disruptions. It appears to be in a relatively stable state, likely past its peak star-forming epoch.
