The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a yellowish hue, suggestive of an older stellar population. Extending outwards from the core, the galaxy shows a faint, bluish envelope, which could indicate the presence of a younger stellar population or ongoing star formation, albeit at a low rate. The galaxy appears elongated, with an approximate axial ratio indicating a moderate degree of ellipticity. There are no obvious signs of major mergers or significant tidal disturbances. Minor perturbations might be present, but the overall structure suggests a relatively relaxed and undisturbed system. The size is relatively compact.
