The galaxy presents as an elliptical morphology. Its overall appearance is smooth and relatively featureless, lacking any discernible spiral arms or prominent dust lanes. The light distribution appears concentrated towards the center, suggesting a dense galactic nucleus. The galaxy exhibits a yellowish-orange hue, possibly indicative of an older stellar population, and comparatively low ongoing star formation. There is no visual evidence to suggest any major mergers or significant tidal disturbances are occurring. The shape is mostly round, with a mild elliptical elongation.
