The galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a centrally concentrated luminosity profile with a bright, possibly older stellar population in the core, indicated by the yellowish hue. The outer regions show a gradual decrease in surface brightness, with a slightly bluer tint suggesting the presence of some younger stars, though this is less pronounced. There may be a faint, disturbed structure near the core, possibly indicating a past interaction or merger event, but the dominant morphology is smooth and spheroidal. No distinct spiral arm features or significant dust lanes are apparent in this observation. The overall shape is generally rounded.
