The galaxy presents as a relatively compact structure. The core region appears smooth and largely featureless with a dominant yellowish-white hue, suggesting an older stellar population. There is minimal evidence of spiral arm structures or significant dust lanes. A slight elongation is discernible, deviating from a perfectly circular morphology. The outer regions exhibit a gradual decrease in luminosity, blending smoothly with the background sky, which may indicate a diffuse halo. The morphology appears generally undisturbed, with no obvious signs of tidal interactions or recent major mergers, though some minor asymmetries cannot be ruled out. Overall, the galaxy appears to be an elliptical or lenticular type.
