The galaxy presents as a relatively smooth, elliptical object. Its light distribution is highly concentrated towards the center, with a gradual decrease in intensity outwards. The galaxy exhibits a roughly circular, but not perfectly round, morphology. There is a subtle color gradient from the center outwards, with a slightly bluer hue apparent in the outer regions compared to the more yellowish core, suggesting some degree of ongoing, albeit subdued, star formation. The overall appearance indicates a system that is not undergoing any major mergers or significant tidal disturbances. The galaxy's morphology is predominantly smooth, with no readily apparent spiral arms or prominent disk structures.
