The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The light distribution suggests a spheroidal structure, possibly an elliptical galaxy, with little evidence of spiral arms or significant dust lanes. The core is bright and compact, indicating a high concentration of stars or possibly an active galactic nucleus. The galaxy exhibits a relatively uniform color gradient, with a slightly bluer hue in the central regions, hinting at a younger stellar population or ongoing star formation, and gradually reddening towards the outer regions, which may contain older stars. The overall shape is nearly circular. There is a lack of significant tidal features or distortions, implying it is not undergoing a major merger event, although minor disturbances cannot be ruled out.
