The galaxy appears as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy seen at a distance where fine details are blurred. It exhibits a slightly flattened shape, verging on round, with a gradual decrease in brightness from the core outwards. The galaxy's color profile suggests a mix of stellar populations, with a predominantly yellowish-white core potentially indicating older stars, surrounded by a bluish halo which may indicate some star formation. There is a possible dust lane or feature bisecting the lower section of the galaxy. There is a hint of some disruption in the outer regions, perhaps indicative of a past or ongoing minor merger event.