The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge with a diffuse, extended halo. The light profile suggests a relatively old stellar population, with a dominant reddish-yellow hue emanating from the core. There is little evidence of strong spiral arm structure or prominent dust lanes. The overall morphology indicates it is likely an early-type galaxy with minimal ongoing star formation. The galaxy's shape is generally round. There does not appear to be any signs of major galactic mergers or tidal disturbances.
