The galaxy presents as a moderately luminous, relatively compact system. The light distribution appears centrally concentrated with a smooth profile, indicative of an elliptical morphology. A subtle color gradient is observed, with a redder core transitioning to a bluer halo. There is a very faint suggestion of a disk component, but the overall structure suggests a more spheroidal configuration. The shape is roughly round. There is no indication of strong tidal disturbances or merging activity, though some faint asymmetries in the outer regions cannot be ruled out as minor disturbances.
