The galaxy presents as a generally smooth, elliptical-like object with a moderate degree of ellipticity. The galaxy exhibits a concentrated central bulge, gradually decreasing in luminosity towards its outer regions. The light distribution suggests a relatively old stellar population throughout the galaxy, but with potential subtle bluer regions closer to the center, which could indicate some ongoing, albeit low, star formation activity. There appears to be little evidence of spiral arm structure or significant dust lanes within this galaxy. The galaxy appears mostly undisturbed morphologically, showing no prominent signs of recent major mergers or tidal interactions. The overall morphology suggests a galaxy in a relatively quiescent state.
