The galaxy presents as a relatively compact, elliptical-like structure. The central region exhibits high luminosity, appearing nearly uniformly bright and smooth across the core. The galaxy is characterized by a general lack of defined spiral arms or a prominent disk. There is a subtle extension of material on one side of the main body, which may indicate a minor disturbance or interaction. The color distribution suggests a population of older stars, with a subtle indication of some ongoing star formation. The overall shape is close to round. There is no obvious evidence of a major merger or significant tidal features.
