The galaxy presents as a centrally concentrated, likely elliptical system. It exhibits a smooth, relatively featureless morphology with no obvious spiral arms or distinct dust lanes visible at this resolution. The core region is noticeably brighter and appears yellowish-orange, potentially indicating an older stellar population. A faint, diffuse halo surrounds the central core, fading gradually into the background sky. The overall shape suggests a high degree of roundness, with a minor elongation or flattening. There is no visually apparent evidence of ongoing major mergers or significant tidal disturbances affecting the galaxy's structure. Faint hints of a disk exist, but it is not the main feature of the galaxy.
