The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated brightness profile, with light intensity gradually decreasing outward from the core. There is no obvious spiral arm structure or prominent dust lanes visible. The galaxy is elongated, but not extremely so, appearing more "in between" round and cigar shaped. There is a subtle color gradient, with the central regions appearing slightly bluer than the outer regions. There are no signs of major disturbances or tidal features suggestive of ongoing mergers, though subtle irregularities are present. The overall appearance suggests a quiescent system with little ongoing star formation.
