The galaxy presents as a centrally concentrated, relatively smooth object, lacking any obvious spiral arm structure. Its overall shape appears to be generally elliptical, with a moderate degree of ellipticity, appearing more "in between" round and elongated. The light profile shows a strong concentration towards the galactic center, indicating a significant bulge component. Color gradients are subtle, with a suggestion of a bluer hue in the outer regions transitioning to a slightly redder core. There is no definitive evidence of ongoing major mergers or tidal disturbances, though minor asymmetries cannot be entirely ruled out.
