The galaxy presents as a largely smooth, elliptical structure with a concentrated, bright central bulge. There is a slight elongation, deviating marginally from a perfectly circular form. Color gradients suggest an aging stellar population, with the core exhibiting a yellow-orange hue, potentially indicative of older, redder stars. A fainter, diffuse halo surrounds the core, fading into the background sky. There may be subtle signs of minor tidal disturbances or interactions, but these are not prominently visible. The overall impression is of a relatively evolved system, consistent with a low star formation rate.
