The galaxy presents as a largely elliptical structure with a smooth, diffuse light distribution. The core region appears brighter and more concentrated than the outer regions. The overall color is yellowish, suggesting an older stellar population. The galaxy exhibits an elongated, but not severely distorted, shape, falling primarily within the 'in between' classification of roundness, indicating a slight deviation from a perfect sphere. There are no clear indications of spiral arms or distinct features suggestive of recent mergers or major disturbances, though a small fraction of the visual classifications suggest minor disturbances. The morphology suggests that it is a fairly relaxed system, potentially evolving towards a lenticular or elliptical form. The galaxy is moderately massive, with low star formation levels.