The galaxy presents a generally smooth, rounded morphology, indicative of an elliptical or lenticular type galaxy. There is a bright central bulge with a concentrated luminosity. The overall color appears to be redder, suggesting a population of older stars. Hints of bluer regions, possibly indicative of more recent, albeit low, star formation activity are visible. There are no discernible spiral arms or dust lanes, and no signs of major merger events, though minor disturbances can not be ruled out. The galaxy appears relatively isolated, lacking close companions or signs of strong tidal interactions.