The galaxy presents as a concentrated elliptical or lenticular structure, exhibiting a high degree of central symmetry. The light profile is smooth and concentrated, diminishing in intensity with increasing radius. It has a rounded morphology. There's no discernible spiral arm structure or prominent dust lanes. The color appears generally consistent, with a possible slight reddening towards the central regions. Based on these characteristics, it is likely a relatively evolved system with a significant spheroidal component. There is no apparent tidal features or distortions indicating recent major merger activity, though some minor disturbances cannot be ruled out given the resolution.
