The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its overall color is a yellowish-white hue, suggesting an older stellar population with fewer young, hot stars. There appears to be only minimal evidence of dust lanes or spiral arm structures. The morphology leans toward an early-type galaxy. There is no obvious sign of any major ongoing merger activity. The galaxy appears fairly isolated with no clear sign of tidal disturbances.
