The galaxy presents a largely smooth and elliptical morphology, appearing somewhat elongated in shape. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. The galaxy displays a color gradient, transitioning from a yellowish-white core to a bluish-green outer halo. This could indicate a population shift from older stars in the core to a slightly younger population in the outer regions. There are hints of minor disturbances in the galaxy's structure, potentially suggesting a past or ongoing interaction with a smaller galactic body, though no significant merging activity is readily apparent in the image. The object appears relatively isolated in the field, which might suggest that any such interactions were historic or that any nearby companions are below the resolution limit. The overall light profile is smooth, showing no evidence of strong spiral arm structures or significant dust lanes.
