The galaxy presents as a somewhat elliptical, lenticular structure, exhibiting a smooth, featureless morphology. A subtle color gradient is observed, with a central region appearing more yellow or golden, potentially indicating an older stellar population, while the outer regions present a slight bluish tinge, suggesting the presence of some younger, hotter stars, or regions of recent star formation. There are no spiral arms or bar structures readily apparent. The galaxy appears relatively undisturbed, with no significant signs of tidal interactions or major mergers. Its overall shape is closer to a rounded form, rather than a highly elongated one. Based on its colors it likely has a moderate mass and moderate rate of star formation.
