The galaxy exhibits a centrally concentrated luminosity profile, suggestive of an elliptical morphology or a spiral galaxy viewed face-on with a dominant bulge. The core region shows a distinct yellowish hue, potentially indicating a population of older, redder stars. The isophotes appear generally smooth, although there is a slight elongation or extension along one axis. A faint, diffuse halo surrounds the brighter central region, gradually fading into the background sky. There is a hint of a tidal feature in the form of a small arm or filament, possibly indicating an interaction with another galaxy. The overall color suggests a relatively evolved stellar population with ongoing, but low-level, star formation.
