The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color appears predominantly yellow-orange, possibly indicating an older stellar population and reduced current star formation. The overall form lacks any prominent spiral arms or distinct features, suggesting a classification towards early-type galaxies. There may be a very faint disk present, but is difficult to see clearly. The galaxy appears to be generally isolated, without obvious signs of recent major merger events or significant tidal disturbances, although there are faint asymmetric features that suggest it may be undergoing minor interactions. The size of the galaxy indicates a substantial stellar mass.
