The galaxy presents as a relatively smooth, lenticular-like structure. It exhibits an overall elliptical morphology, with a noticeable central bulge, though some disk-like features are apparent with slight distortions. The color profile suggests an older stellar population, with yellow to red hues dominating the central regions indicating diminished star formation, while bluer edges hint at younger stars in the outskirts. There is evidence of potential interaction or merging activity, with the possibility of minor disturbances in the surrounding areas. The galaxy seems to be of intermediate mass.
