The galaxy presents as a centrally concentrated, generally smooth object with an elliptical morphology. The central region exhibits a bright, slightly yellow-tinged glow, potentially indicating a concentration of older stellar populations. The outer regions appear more diffuse, fading into the background sky. There may be a faint hint of a disk-like structure or spiral arm segment. There is no obvious evidence of strong tidal interactions or ongoing major mergers. It does appear to be a generally isolated galaxy.
