The galaxy presents a predominantly smooth and rounded morphology. The light profile indicates a centrally concentrated object with a noticeable fall-off in surface brightness away from the core. Color gradients are subtle but suggest a slightly bluer hue in the outer regions compared to the yellower core, potentially indicative of ongoing star formation in the outer parts. There is no apparent disk structure or spiral arm morphology. Evidence for any major merging events is absent, and no tidal tails or significant disturbances are visible. The overall impression is that of a relatively undisturbed, mature system.
