The galaxy presents as a centrally concentrated elliptical-type system. Its overall form is elongated, appearing cigar-shaped in its projection on the sky. The light distribution is smooth, with no prominent spiral arms or significant disk-like features readily apparent. The central region exhibits a slightly reddish hue, indicative of a population of older stars or dust obscuration. A more diffuse, bluish halo surrounds the core, possibly suggesting the presence of a younger stellar population at larger radii, or potentially a shell-like structure. There are no obvious signs of tidal disturbances or ongoing mergers; the galaxy's morphology appears relatively undisturbed.
