The galaxy presents an elongated, elliptical morphology. It appears largely smooth and centrally concentrated, with the light profile gradually decreasing outwards from a bright core. The color distribution suggests a relatively evolved stellar population; the central region exhibits a yellowish-white hue, potentially indicative of older stars. The outer regions of the galaxy have a bluish tint, suggesting some level of ongoing or recent star formation activity, though this is much less pronounced than the central region. There is no readily apparent disk structure or spiral arm features. No major morphological distortions are detected; however, there may be a minor perturbation in the outskirts of the galactic halo.
