The galaxy presents as a smooth, elliptical object. It exhibits a concentrated, bright central bulge that gradually diffuses outwards. The morphology suggests it is generally cigar-shaped. The colour gradient shows a slightly yellower core transitioning to bluer hues in the outer regions, suggesting a distribution of stellar populations with possibly older stars towards the center and younger stars in the outer regions. There may be a slight disturbance in its structure, though its overall appearance is consistent with a relatively undisturbed system. The overall form does not indicate any ongoing major merging activity.
