The galaxy presents as a moderately luminous elliptical morphology. The core exhibits a bright, concentrated central bulge, with a yellow-orange hue suggestive of an older stellar population. There is a gradual decrease in luminosity outward from the core, transitioning to a more diffuse, indistinct halo. The overall shape is cigar-shaped, with a slight elongation along one axis. There is no evidence of distinct spiral arms or significant dust lanes within the galaxy's structure. The smooth texture is indicative of a dynamically relaxed system. There are no signs of major tidal disturbances or ongoing mergers, although minor irregularities cannot be excluded at this resolution.
