The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and rounded morphology. Its overall color is a yellow-red hue, which suggests a stellar population dominated by older, redder stars and potentially a lower rate of on-going star formation. There appears to be a bright central bulge, with a more diffuse halo or outer region extending from it. There are no easily discernible spiral arms or prominent dust lanes. The galaxy shows no obvious signs of major disturbances, strong tidal features, or recent merger activity. Close inspection does reveal some very minor disturbances within the galaxy's outskirts.
