The galaxy appears to be a relatively compact elliptical or lenticular galaxy, exhibiting a smooth, centrally concentrated luminosity profile.  The core region is a bright, yellowish-white, suggesting a population of older stars. There's a gradual decrease in surface brightness moving outward from the center, with the outer regions appearing more diffuse and slightly bluer in color, implying the presence of a small fraction of younger stars or ongoing low-level star formation. No distinct spiral arms or bar structures are discernible. The overall shape is largely circular, exhibiting little to no apparent elongation or tidal features that would indicate a recent major merger. There are only hints of minor disturbances in its structure.
