The galaxy presents a relatively smooth, elliptical morphology. It is somewhat centrally condensed with a diffuse halo. The primary light source is the bulge, with no distinct features visible. The galaxy appears to be relatively isolated, showing no obvious signs of major mergers or significant tidal disturbances. There appears to be a slight asymmetry within the overall light distribution, but more data would be needed to determine the cause. The color suggests a mature stellar population, with minimal recent star formation.
