The galaxy presents as a centrally concentrated object with a smooth, generally elliptical morphology. The core exhibits a bright, yellowish hue, indicating a population of older stars. There is little evidence of distinct spiral arms or significant dust lanes within the visible structure. The galaxy appears relatively undisturbed, without major signs of tidal interactions or ongoing mergers. The observed color suggests the presence of a stellar population that is not actively forming stars at a high rate. The galaxy appears somewhat rounded, with no significant elongation. There are no noticeable features indicating a highly disturbed or actively merging system, though a slight asymmetry cannot be fully ruled out.
