The galaxy presents as a single, centrally concentrated object with a generally smooth profile. There appears to be little to no discernible spiral structure or distinct features such as bars or rings. The galaxy exhibits an elliptical shape. The core region displays a yellowish-white hue, suggesting a population of older stars, whereas the outer regions of the galaxy appear subtly bluer, potentially indicative of more recent star formation activity. No obvious signs of a major merger or significant tidal disturbances are visible. A slight asymmetry in the outer envelope might indicate a minor past interaction. The object appears largely undisturbed with a fairly regular morphology.
