The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in surface brightness moving outward from the core. The galaxy appears nearly round. There are no prominent spiral arms or obvious features indicating ongoing mergers. The overall color suggests a population of older stars, with a relatively low star formation rate. The galaxy's red color indicates that it consists of older stars as well, and therefore is likely in the red sequence. 
