The galaxy presents an overall elliptical morphology. The core region exhibits a smooth, concentrated light profile, suggestive of an older stellar population. There is a slight disclike asymmetry extending to the left from the center. The light from the left has a yellowish to orangish color suggesting it contains older stars and dust. To the right of the main body of the galaxy, there is a bright blue region, which could be a population of young, hot stars. The galaxy appears relatively isolated and has a smooth structure with low tidal disturbances, this may indicate the galaxy is not currently undergoing a major merger.
