The galaxy presents as a single, though not perfectly round, object. Its color appears to be trending from yellow to red. The galaxy exhibits a fairly homogenous profile. There is no evidence of significant spiral arm structure, or a defined nucleus. A smooth profile is noted. There is no visual evidence of a recent major merger. The galaxy's color suggests ongoing star formation, with indications of both young, hot stars and a population of older, redder stars. The apparent smoothness and lack of pronounced features could be indicative of an elliptical galaxy, or potentially a spiral galaxy viewed at an angle that obscures its spiral structure.
