The galaxy presents as a single, relatively symmetrical, and concentrated object. It has a smooth, amorphous appearance with no readily discernible spiral arms or bar structure. The central region exhibits a brighter, yellowish-white hue, suggestive of an older stellar population. The outer regions gradually fade into a bluish halo, potentially indicating the presence of a younger stellar population or ongoing star formation at the edges, though faint. The galaxy’s overall shape is more or less circular, indicating that it could be an elliptical galaxy or a spiral galaxy viewed face-on without substantial disruption from mergers. There is no obvious sign of tidal tails, strong asymmetries, or other features indicative of an ongoing or recent major merger event.
