This galaxy presents as a relatively smooth, elliptical-like structure. It appears elongated, with a cigar-shaped morphology, suggesting it is not perfectly spherical. The primary color is a yellowish-orange hue, which could indicate an older stellar population and lower levels of on-going star formation. There are very faint hints of bluer regions within the disk, but the overall color indicates that the galaxy may be composed mostly of older stars. The disk is relatively undisturbed with no clear indication of major mergers or significant tidal distortions.
