The galaxy appears as a centrally concentrated, yellowish-orange object. Its morphology is generally smooth and elliptical, with no discernible spiral arms or distinct features such as dust lanes or star-forming regions visible in the current resolution. The light distribution indicates a relatively even luminosity gradient extending from the central core to the outer edges, suggesting an older stellar population dominating the galaxy's composition. The object presents a moderate ellipticity, leaning more towards a round shape than a highly elongated form. There is no obvious indication of tidal interactions or ongoing merging activity, although subtle disturbances might be present at a scale beyond the detection limit of this image.
