The galaxy appears to be a relatively smooth, elliptical-like structure. The light profile is concentrated towards the center, with a gradual decrease in brightness moving outwards. It exhibits a yellowish-golden hue, indicating a population of older stars. There is no strong evidence of spiral arms or significant dust lanes from what is visible, and no obvious signs of recent major merger events. Minor disturbances cannot be ruled out, as the features are not well defined with this resolution. It appears round.
