The galaxy presents as a generally smooth, elliptical object with a concentrated central bulge. It exhibits a radial color gradient, appearing yellow-white at the core, gradually transitioning to a redder hue in the outer regions. There is no apparent spiral arm structure or prominent dust lanes are visible. The galaxy appears largely undisturbed, with no obvious signs of ongoing mergers or major tidal interactions. The light distribution is highly concentrated, which implies that it is very likely a high mass galaxy. The moderate red shift indicates that it is at a cosmologically significant distance. The overall color suggests that this is a relatively old galaxy dominated by an older stellar population with a relatively low specific star formation rate.
