The galaxy presents as a relatively smooth, elongated, and cigar-shaped structure. Its core exhibits a concentrated luminosity, appearing yellowish-orange, indicative of an older stellar population. Surrounding the core, a fainter, bluer halo is observed, hinting at the presence of some younger stars or ongoing star formation activity, albeit at a subdued level. There's no clear evidence of spiral arms or a distinct disk. Faint irregular shapes extend away from the central region on either side of the galaxy.
