The galaxy presents as a generally smooth and rounded structure, suggestive of an elliptical morphology. A concentrated central bulge is apparent, exhibiting a yellow-orange hue, possibly indicating an older stellar population. Fainter, less defined extensions are seen surrounding this core, blending gradually into the background sky. These extensions appear smoother and more diffuse. There may be some indication of minor disturbances or interactions, but overall the galaxy appears relatively undisturbed.
