The galaxy presents as a moderately luminous, elliptical system. It exhibits a smooth, centrally concentrated light profile with a gradual decrease in luminosity moving outward from the core. The core region is a yellow-white hue, indicative of an older stellar population dominated by red giant stars. The galaxy appears somewhat flattened, displaying a more lenticular morphology. There is a hint of a very faint, diffuse disk, but no distinct spiral arm structure is visible. No significant dust lanes or prominent star-forming regions are apparent. There is a lack of blue light, implying there is little ongoing active star formation. The surrounding halo appears sparse, and there does not appear to be any tidal features or signs of recent major mergers. The galaxy exhibits a relatively undisturbed morphology.
