The galaxy appears as a single, relatively smooth object with a centrally concentrated light profile. It displays an elliptical morphology, appearing more "in between" round and cigar shaped than either. There is a slight blue hue to the galaxy, suggesting some recent or ongoing star formation activity, even though the majority of the light appears consistent with an older stellar population. No significant dust lanes, spiral arms, or bar features are readily apparent. The overall structure suggests a galaxy that has largely completed its major merging history, with no signs of major disturbances or ongoing merger events. The light is centrally condensed, without distinct clumps or irregularities, indicating an undisturbed and settled system.
