The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits an elliptical shape. A bright, yellowish core region is present, suggesting a high density of older stellar populations. Fainter, bluer light surrounds the core. Overall it is a relatively compact object. There is no indication of spiral arm structure or major morphological disturbances; subtle irregularities in the outer regions might suggest minor interactions or internal structures, but this is not definitive from the available image. The object's radial color gradient indicates a likely change in stellar population from the center to the outskirts.
