The galaxy presents as a primarily smooth, elliptical structure, exhibiting a concentrated central bulge that transitions smoothly into a fainter, more diffuse outer halo. There is a slight elongation. Color gradients suggest some internal structure; a yellowish-white hue dominates the central region, potentially indicative of an older stellar population. The outer regions display a hint of bluer tones, suggesting the presence of some younger, hotter stars or ongoing star formation, though minimal. The overall morphology is largely undisturbed, with no obvious signs of major mergers or tidal interactions.
