The galaxy presents as a relatively compact, smooth object with a dominant central bulge. The morphology suggests a likely elliptical or S0 type galaxy. A subtle color gradient is observed, with the core exhibiting a yellowish hue transitioning to a slightly bluer tint in the outer regions. This could indicate older stellar populations concentrated within the nucleus. The galaxy appears undisturbed with no signs of recent mergers or tidal features. The overall structure implies a dynamically relaxed system.
