The galaxy presents as a diffuse, yellowish-white structure with an apparent elliptical morphology. The central region is significantly brighter and more concentrated, suggesting a prominent bulge. A fainter, more extended halo surrounds the central region, with a subtle disk-like feature visible to the southeast. This disk shows indications of internal structure, possibly spiral arms or dust lanes, exhibiting a slightly redshifted color. There is a suggestion of a merging event or tidal disturbance, given the irregular shape and asymmetries in the outer regions of the galaxy. The galaxy's overall color indicates a population of older stars, but the bluer region in the southeast suggests ongoing star formation.
