The galaxy presents a primarily smooth, elliptical morphology, with minimal evidence of spiral arm structure. It exhibits a moderately concentrated central bulge that appears approximately circular in projection. The color gradient suggests a population of older stars, possibly indicating a relatively quiescent star formation history. Faint, extended halos of diffuse light surround the main body, and a small number of slightly asymmetrical features may suggest minor tidal interactions or recent accretion events, although this is difficult to discern. There are no distinct dust lanes or prominent star-forming regions visible.
