The galaxy presents as a centrally concentrated object with a roughly elliptical morphology, exhibiting a smooth luminosity profile suggestive of an early-type galaxy. There is a pronounced central bulge characterized by a yellowish-white hue, possibly indicative of an older stellar population. The outer regions of the galaxy gradually fade into the background sky, showing a diffuse and unresolved structure. There is no apparent spiral arm structure or prominent dust lanes visible. The overall color is relatively red, which could indicate a relatively low rate of ongoing star formation. Slight asymmetric features may be indicative of past or ongoing minor interactions or disturbances, though the dominant impression is of a relatively undisturbed and evolved system.
