The galaxy presents as a cigar-shaped structure, significantly elongated along its major axis. The central region exhibits a brighter, more concentrated luminosity, indicative of a galactic bulge. The light profile appears relatively smooth, though some faint, diffuse features hint at a possible disk. The colour gradient shifts from a bluer hue within the central region to a redder tone towards the outer edges, potentially signifying differing stellar populations and active star formation in the central region. The overall morphology appears largely undisturbed. There are no clear indications of ongoing major mergers or strong tidal interactions within the system.
