The galaxy presents as a somewhat smooth, centrally concentrated structure. Its overall shape appears elliptical, but is close to being round. There is a bright central bulge region, which fades gradually into a less luminous, diffuse halo. Some faint, irregular features or disturbances can be discerned in the outer regions, possibly suggestive of minor interactions or internal processes. The galaxy exhibits a color gradient, with the central regions appearing more yellow/white, potentially indicating an older stellar population, while the outer regions show hints of bluer hues, suggesting the presence of younger stars or ongoing star formation. However, the overall color is redder than more active star-forming galaxies, suggesting a moderate degree of star formation activity. There is no clear indication of spiral arms or a prominent disk structure.
