The galaxy presents as a relatively smooth, elliptical or lenticular object. It displays a concentrated central bulge that is significantly brighter than the surrounding halo. The galaxy exhibits a fairly regular, round morphology. The light distribution appears mostly uniform, with no readily apparent spiral arm structures or strong dust lane features visible. There are no visual indications of a major ongoing merger event or significant tidal disturbances. Subtle color variations are present, with the core showing a yellower hue suggestive of an older stellar population, while the outer regions seem slightly bluer, possibly indicating regions of younger stars, though this is marginal. Overall, the galaxy appears to be a mature system, likely dominated by relatively old stars and a quiescent star formation rate.
