This galaxy exhibits a smooth morphology, appearing largely spheroidal in shape. It presents as a singular object with what may be a possible merging structure. This appears to be a relatively old system, where current star formation is not dominant. The galaxy displays a yellowish to reddish hue, which indicates a population of older stars, and is not particularly elongated. There is no apparent dust lane or spiral arm structure. The overall appearance suggests a system undergoing a possible merging event, however, it mostly appears as a well-formed system undergoing minor disturbances.
