The galaxy appears as a centrally concentrated object with a generally smooth profile. It exhibits a nearly circular morphology, lacking any obvious strong distortions or asymmetries. The core is a bright yellowish-white, suggesting an older stellar population. There is a gentle fall-off in light intensity from the center outwards. The outer regions display a slight bluish-white tint and are faint, potentially indicating the presence of a younger stellar population, though this is not definitive from the image alone. No spiral arm structures or significant dust lanes are discernible. The overall appearance is that of a relatively undisturbed system, with no apparent ongoing major mergers or tidal interactions.
