The galaxy presents as a fairly smooth, elliptical-like structure. It displays a centrally concentrated bulge that is more luminous than its surrounding areas, with a gradual decrease in surface brightness as one moves outward. The galaxy does not show any obvious spiral arm structures or prominent dust lanes. Its color appears to be a relatively homogenous blue-white, indicating the presence of a moderate population of relatively young stars. There is no evidence of a major ongoing merger, although it does have slight irregularities. The overall morphology suggests that it is most likely a mature galaxy undergoing slow star formation. The estimated size is approximately 3.6 kiloparsecs.
