The galaxy presents as a relatively compact object. Its morphology appears largely smooth and centrally concentrated with hints of disk-like features. Color gradients indicate a possible transition from a bluer, potentially younger stellar population in the core to redder, older populations in the outer regions. The overall roundness is in between round and cigar shaped. There is no strong visual evidence of ongoing major mergers or significant tidal disturbances, though minor disturbances cannot be completely ruled out. The integrated light suggests a relatively massive galaxy.
