The galaxy appears as a centrally concentrated, relatively smooth structure with a dominant, ellipsoidal morphology. The light distribution suggests a lack of significant spiral arm structures or prominent dust lanes. The galaxy exhibits a yellowish-white color, indicative of an older stellar population, potentially dominated by evolved stars. There are hints of some internal structure, but it lacks any sharp or well-defined features. The overall impression is one of a mature galaxy that has undergone significant dynamical relaxation. The galaxy does not seem to be undergoing any major mergers, but there are subtle indications of disturbances.
