The galaxy presents as a single, concentrated object with a smooth light distribution. The core is bright and gradually fades outward without any distinct spiral arm structures, prominent dust lanes, or knotty star-forming regions discernible. The shape is somewhat elliptical, approaching round, though a slight elongation is observed. The color appears yellowish-orange, suggesting a dominant population of older stars and relatively low current star formation activity. There is a suggestion of a minor tidal disturbance, or a faint, diffuse feature extending slightly from the galaxy's main body, potentially indicative of past interactions or ongoing minor mergers.