The galaxy presents as a somewhat elongated, elliptical morphology. There is a smooth, concentrated central bulge that transitions into a more diffuse outer region. The color profile appears to be generally redder in the central regions, suggestive of an older stellar population, while the extremities exhibit bluer tones. This could indicate younger stars or ongoing star formation in the outer regions, or it could be caused by noise in the image. There is no discernible dust lane or spiral structure visible, based on the optical data. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal disruptions. There is a faint, diffuse halo surrounding the main body of the galaxy.
