The galaxy presents as a smooth, centrally concentrated object. The core exhibits a bright, yellow-orange hue, indicative of an older stellar population. There's minimal evidence of spiral arm structure, suggesting either an elliptical morphology or a face-on spiral with a dominant bulge. The outer regions of the galaxy fade gradually into the background, showing no sharp edges or distinct features. The overall shape appears nearly round, with a slight elongation. There are no obvious signs of tidal disturbances or ongoing mergers, implying a relatively quiescent state.
