The galaxy appears as a relatively smooth, centrally concentrated object. Its overall shape is close to circular. There is a prominent central bulge of yellowish-white light. The color distribution suggests a lack of significant dust lanes or spiral arm structures. It has a relatively high degree of smoothness, with little evidence of ongoing or recent major merger activity. The galaxy exhibits colors indicative of an older stellar population and a relatively quiescent star formation rate. There are no clear indications of tidal tails or disrupted morphology. The galaxy appears relatively isolated.
