The galaxy appears as a single, relatively smooth and centrally concentrated object. There is an apparent lack of distinct spiral arms or a prominent bar structure. The morphology suggests a likely elliptical or lenticular galaxy type, displaying a high degree of rotational symmetry. The light profile appears to be smoothly distributed, indicative of an older stellar population. There is a possible presence of some minor disturbances in the outer regions, but these are not indicative of a major ongoing merger event. It exhibits a round morphology, lacking a significant cigar shape, so it can be considered almost circular. The galaxy's color is somewhat yellow, suggesting a population of older stars.
