The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a concentrated central bulge that gradually fades into a more diffuse outer region. There's a hint of a flattened disk-like structure, but it is not strongly defined. The galaxy appears to be relatively isolated, with no obvious signs of ongoing major mergers or tidal disturbances. The primary color is a yellowish-red hue, suggesting an older stellar population with low ongoing star formation, though some bluer regions indicate localized star formation. The overall symmetry and smooth light profile suggest a dynamically relaxed system. There may be spiral arms that are difficult to differentiate from the rest of the galaxy.
