The galaxy presents as a relatively smooth and compact object. It appears largely elliptical in shape, with a central bulge that is bright and dominant. A diffuse halo surrounds the central region, showing a gradual decrease in luminosity towards the outer edges. There's some faint evidence of a disk-like structure, though it's not sharply defined. Possible minor disturbances are visible, suggesting a recent or ongoing interaction or accretion event. The galaxy does not appear to be undergoing a major merging event, but shows hints of possible minor disturbances. Color gradients suggest a mix of stellar populations, with the central bulge possibly hosting older, redder stars, while the outer regions may contain younger, bluer stars indicative of ongoing or recent star formation. Overall, the galaxy seems to be an intermediate-mass system displaying characteristics of both early and late-type galaxies.
