The galaxy presents a primarily smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with brightness decreasing gradually towards the outer regions. The galaxy appears relatively isolated, with no obvious signs of major mergers or strong tidal interactions with neighboring galaxies, though some minor disturbances cannot be ruled out. There is a very slight potential for a faint, diffuse structure. The colors observed are indicative of an older stellar population, with a redder overall hue, although there is some presence of bluer light concentrated in the center of the galaxy. The galaxy is relatively compact in size.
