The galaxy presents a generally smooth, elliptical morphology. The overall color profile appears consistent with an older stellar population, showing a yellowish hue. The galaxy is relatively concentrated, with no obvious spiral arm structures or significant dust lanes visible. There is a slight deviation from perfect circularity; the shape is somewhere between round and slightly elongated. There are some indications of a minor disturbance or interaction, but it could be a result of its shape. Overall, the galaxy appears to be relatively quiescent, showing little evidence of significant star formation activity.
