The galaxy presents as an elliptical or lenticular type, characterized by a generally smooth and diffuse light distribution. There's a pronounced central bulge that appears to be dominated by older stellar populations, indicated by its yellowish-orange hue. The galaxy exhibits a slight elongation, with a relatively indistinct disk component. No spiral arm structures are clearly discernible. Overall, the galaxy does not show strong evidence of recent major mergers or significant tidal disturbances; however, a mild asymmetry could suggest minor gravitational interactions. The galaxy shows low star forming activity, as indicated by the colors.
