The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile is concentrated towards the center, with a gradual decrease in intensity outwards. A mostly uniform color distribution suggests an older stellar population and subdued star formation activity, this is further supported by the mostly redder color profile. There is no evidence of strong spiral arms, bars, or tidal features, suggesting that the galaxy is not currently undergoing a major merger or significant interaction with other galaxies. The galaxy appears quite round overall, without any significant elongation or distortion.
