The galaxy presents as a generally smooth, elliptical structure. It exhibits a bright, concentrated central bulge that appears roughly spherical, gradually fading into an extended halo. The halo seems to be more elongated and elliptical than the central bulge, giving the galaxy an overall lenticular shape. The light distribution within the galaxy appears relatively uniform and lacks prominent spiral arms or dust lanes, suggesting an older stellar population. The color of the galaxy is generally yellowish-orange, indicative of a population dominated by older, redder stars. There may be some subtle bluer regions hinting at pockets of more recent star formation, but the overall star formation rate appears low. There is some visual evidence of a minor tidal disturbance or a possible interaction with a small companion galaxy, observable as a faint extension or asymmetry on one side of the main galactic body. This suggests a possible merger event in the galaxy's history. The overall impression is of a fairly massive, evolved galaxy undergoing a relatively quiescent period in its evolutionary history.
