The galaxy presents a somewhat disturbed morphology, appearing as an elliptical structure with a possible minor disturbance or merger event in progress. The main body exhibits a smooth appearance, but there is evidence of a secondary, less defined component seemingly interacting with the primary structure. The overall shape deviates slightly from a perfect ellipse, hinting at tidal distortions or ongoing interactions. There is a single bright, concentrated center that accounts for most of the light being emitted from the galaxy. Color gradients suggest a population of older stars, with a reddish-yellow hue dominating the galaxy. Star formation appears to be relatively quiescent within the main body, with no obvious concentrations of blue light indicating active regions. The galaxy does not present a spiral disk.
