The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, centrally concentrated light profile. The light is more concentrated in the center than the outer parts of the galaxy, meaning the galaxy is more yellow and red in the center than the outer parts. The smooth distribution of light suggests an older stellar population with less active star formation. There is evidence of a faint, diffuse halo extending beyond the central core. The axial ratio is close to unity, suggesting a nearly circular morphology when viewed from our vantage point. There appear to be no signs of recent major mergers or tidal disturbances, indicating the system is relatively undisturbed. There could be some minor disturbance, but nothing visible with the information given.
