The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a generally round morphology, with a slight deviation towards a more oblate spheroid than a perfect sphere. The color profile suggests a predominantly older stellar population, with a yellow-red hue dominating the central bulge. There is little to no evidence of spiral arm structures or prominent dust lanes. The galaxy is quite compact, with light appearing centralized and diminishing gradually from the core outwards. There is a faint suggestion of a diffuse halo, with color becoming slightly more blue than the yellow center of the galaxy. There are no obvious signs of a recent major merger event.
