The galaxy presents a generally smooth and elliptical morphology, with a highly concentrated central bulge exhibiting a yellowish-orange hue. This central region appears to be comprised of an older stellar population. Moving outwards from the center, a diffuse disk is observed, displaying a bluer tint, suggestive of ongoing or recent star formation. While the disk is present, it lacks distinct spiral arm structures or prominent dust lanes; its features are generally subtle. The overall shape appears largely undisturbed, with no obvious signs of major tidal interactions or ongoing mergers. Minor asymmetry may be present in the outer regions of the disk, indicating potential subtle gravitational interactions or disturbances. The galaxy exhibits a moderate redshift, suggesting it is at a considerable distance.
