The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile is centrally concentrated, with a bright, yellowish core gradually fading into a more diffuse halo. The isophotes appear elongated, suggesting a moderate degree of ellipticity. There is little indication of spiral arm structure or prominent dust lanes. The overall color is moderately red, suggestive of an older stellar population with lower levels of ongoing star formation. Faint, bluish regions are seen scattered throughout the galaxy. There is no sign of strong tidal disturbances or ongoing mergers.
