The galaxy presents as a largely smooth, elliptical-like structure. There is a central bulge that dominates the galaxy's light profile. The core exhibits a yellow-white hue, indicative of an older stellar population. The outer regions show a gradual decrease in surface brightness, fading into the background sky. There is no readily apparent spiral arm structure or significant dust lane features. A very slight asymmetry might be present, but it is not possible to conclusively assess the presence of tidal features or signs of recent merging activity from this image alone. The galaxy appears relatively isolated. The colors imply low to moderate levels of star formation.