The galaxy presents a generally smooth morphology, appearing largely elliptical. The light distribution is concentrated towards the center, with a gradual decrease in intensity outward. There is a slight elongation. The galaxy exhibits a yellow-red hue, suggestive of an older stellar population. There is no obvious dust lane, spiral arm structure, or prominent star-forming regions. The overall impression is that of a relatively quiescent galaxy. There appears to be a slight hint of asymmetry in its outer regions which could suggest a prior minor merger.
