The galaxy presents as a smooth, centrally concentrated object, most likely an elliptical galaxy given its lack of apparent spiral arms or a distinct disk. The light profile is generally spheroidal, with a gradual decrease in brightness from the core outwards. The galaxy exhibits a yellowish-orange hue, suggesting an older stellar population and a relative lack of ongoing star formation. There is a slight elongation to the galaxy, but it is generally round in appearance. No obvious tidal features or signs of recent or ongoing major mergers are observed, though subtle disturbances cannot be ruled out. The galaxy appears relatively isolated within its immediate vicinity.
