The galaxy exhibits a generally smooth morphology, with a high degree of roundness to its overall shape. There is no distinct spiral arm structure visible; the light is rather diffuse and centrally concentrated. The color appears to be slightly reddish, which could be indicative of an older stellar population with less active star formation. There is no obvious evidence of a major merger or tidal disturbances, although a minor disturbance or interaction cannot be completely ruled out based on this image alone.
