The galaxy presents as a somewhat elliptical, although potentially disk-like, structure viewed at an oblique angle. It exhibits a relatively smooth appearance, with a concentrated central bulge region that is slightly brighter than the surrounding disc. The overall color is slightly yellowish-white, suggestive of a population of older stars and a relatively low star formation rate. Faint indications of potential disturbances are visible in the outer regions, possibly indicating past or ongoing minor interactions with smaller companion galaxies.
