The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated core that transitions into a more diffuse halo. The overall color appears to be consistent with an older stellar population, suggesting minimal ongoing star formation within the galaxy. There is no apparent spiral arm structure or dust lane features visible. The galaxy seems largely undisturbed, with no obvious signs of any major merger events or tidal interactions. A slight elongation is seen in the morphology, but it remains largely spheroidal.
