The galaxy presents a generally smooth, elliptical morphology. The light is centrally concentrated with a gradual decrease in surface brightness moving outwards from the core. The core exhibits a yellow-orange hue, possibly indicating an older stellar population. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or recent mergers. There is a very faint hint of a possible disk or faint structure surrounding the bulge, although difficult to discern. The galaxy's overall color suggests an older population of stars. Star formation appears to be minimal. It appears to be a relatively massive system.
