The galaxy presents a centrally concentrated light profile, suggestive of an elliptical or lenticular morphology. The central region appears smooth and rounded. There is a faint, diffuse halo extending beyond the core, with a slight elongation observed in the upper right direction. The overall color is yellowish-orange, which indicates an older stellar population with minimal ongoing star formation, in other words, redder colors tend to imply older stars. There may be a very slight hint of disturbance or asymmetry in the outer regions.
