The galaxy presents as a centrally concentrated, relatively smooth structure, with a general elliptical morphology. A subtle color gradient can be observed, transitioning from a bluish hue in the central region to a redder periphery. There is faint indication of a possible disk-like structure or spiral arm feature within the fuzziness, which will require a higher resolution image for any more certain confirmation. The roundness is mostly in between fully circular or elongated. There appears to be only minor signs of disturbance or tidal features, suggesting relative gravitational equilibrium. Star formation is present, but at a modest rate. The galaxy exhibits a notable level of luminosity. The spatial extent is relatively compact.
