The galaxy presents as a relatively smooth, elliptical morphology with an apparent lack of distinct spiral arms or features. It exhibits a concentrated central bulge that transitions gradually into a more diffuse halo. Color gradients are subtle, with a yellowish hue in the core region suggestive of an older stellar population, possibly dominated by red giant stars. The outer regions appear bluer. This may be due to a smaller population of younger, hotter stars or a low level of ongoing star formation. There is no obvious evidence of a recent major merger event, although the possibility of a past interaction cannot be ruled out based on this image alone. The galaxy appears fairly undisturbed. The overall shape leans towards being in between round and elliptical.
