The galaxy presents as a primarily elliptical structure, exhibiting a concentrated central bulge that emits a yellow-orange hue. The core region appears smooth, suggesting an older stellar population is dominant. A fainter, bluer disk component is visible beyond the bulge. The galaxy's overall light profile is relatively smooth, with subtle indications of internal structure. The disk is somewhat disturbed, possibly exhibiting minor tidal interactions or internal asymmetries. There is no strong evidence for on-going major mergers or active starburst activity, though some star formation could be present.
