The galaxy appears as a somewhat diffuse object, exhibiting a centrally concentrated morphology. The core region presents a distinct yellowish-orange hue, suggesting a population of older stars and potentially dust obscuration. The surrounding halo displays a bluer tint, indicative of a younger stellar population and possible ongoing star formation. The galaxy appears to be relatively undisturbed with no strong signs of tidal interactions or major mergers. The overall shape appears to be somewhere between elliptical and disk-like with no clear spiral arm structures visible.
