The galaxy presents as a somewhat elongated, lenticular structure with a smooth, diffuse appearance. The central bulge exhibits a concentrated luminosity, displaying a yellowish-orange hue suggesting an older stellar population. There are no prominent spiral arm features visible. The outer regions appear fainter and more diffuse, gradually blending into the background sky. The overall color gradient indicates a possible lack of significant recent star formation activity. There is slight evidence of possible gravitational disturbance, in the form of a warped disk.
