The galaxy presents as an elliptical or lenticular type. It exhibits a relatively smooth, centrally concentrated light distribution, with a gradual decrease in luminosity towards the outer regions. The core appears bright and slightly yellowish, potentially indicating an older stellar population. There is a subtle elongation visible but no strong bar feature. The overall morphology indicates a galaxy that has largely completed the process of hierarchical assembly and has likely exhausted much of its gas reservoir for active star formation. Hints of a faint, diffuse halo structure are visible, extending beyond the main body of the galaxy, but no distinct spiral arm structure.
