The galaxy presents as a somewhat elliptical, extended object with a generally smooth appearance. The central region exhibits a high degree of luminosity, appearing nearly spherical. A fainter, more diffuse halo surrounds the central bulge, extending primarily along the horizontal axis of the image. Faint hints of asymmetry are visible within the outer regions of the halo, suggestive of tidal disturbances or ongoing interactions.

The color profile indicates a population of older stars, particularly within the central regions, exhibiting a redder hue. The outer disk shows subtle bluer tinges, hinting at the presence of younger stellar populations. The overall color distribution, and hints of asymmetry, suggests a possibility of recent or ongoing minor merger events.
