The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a centrally concentrated luminosity profile. Its overall shape is somewhat rounded. There is no obvious presence of spiral arms or a distinct disk component. The color indices indicate a relatively passive stellar population, possibly dominated by older stars. There might be minor disturbances in the structure of the galaxy, but no signs of major mergers or strong tidal features are apparent. The estimated size suggests it is an intermediate size galaxy. The galaxy's low star formation rate is consistent with its morphology and colors.