The galaxy presents an elliptical morphology. It exhibits a smooth, relatively featureless profile, with no apparent spiral arms or a prominent central bar. The light distribution is centrally concentrated, indicating a likely evolved stellar population dominating the core. Color gradients are observed, with a yellowish-white hue in the central regions, gradually transitioning to bluer tones in the outer halo. The observed color suggests ongoing, albeit moderate, star formation activity. No signs of major mergers or significant tidal disturbances are apparent. The galaxy appears to be in a relatively relaxed state.
