The galaxy presents as a centrally concentrated object, appearing generally smooth in morphology. It exhibits an elliptical shape, although it tends towards roundness rather than being highly elongated. The light profile appears to decrease gradually from the core outwards. A slight color gradient can be observed, with the central region appearing yellowish-white, potentially indicative of an older stellar population. Fainter, bluer tinges are present in the outer regions of the galaxy, which may imply more recent or ongoing star formation. There is no obvious presence of spiral arms or a distinct disk structure. There is no major ongoing merger or major disturbance, although it appears the galaxy could be experiencing some minor disturbances to its structure.
