The galaxy presents as a generally smooth, centrally concentrated object with an elliptical morphology. A bright, yellowish core dominates the central region, indicative of an older stellar population. Moving outwards from the core, a gradual transition to a more diffuse, bluish halo is observed. Hints of subtle, disturbed structures and faint spiral arms are seen, but could also be a merger remnant. The overall structure appears relatively undisturbed, but it may have experienced a recent minor interaction. The object exhibits a moderate level of star formation, as evidenced by the blue color within the fainter outer regions.
