The galaxy presents a smooth, elliptical morphology. It is elongated in shape, appearing cigar-like. The central region exhibits a high surface brightness, with a gradual decrease in luminosity towards the outer edges. There is a subtle disk-like structure, but it is very diffuse and faint. There does not appear to be any strong evidence of significant tidal disturbances or ongoing major merger activity. The colour profile indicates a dominance of older stellar populations. There are no visible prominent dust lanes or spiral arms.
