The galaxy presents as a somewhat elliptical, disk-like structure, viewed at a significant angle relative to face-on. A bulge is present, appearing centrally concentrated and slightly elongated along the major axis. The disk component is visible as a flattened extension on either side of the bulge, with hints of spiral arm structure.

Color variations are present throughout the galaxy. The central bulge appears more reddish, which could indicate an older stellar population and dust obscuration. The outer disk regions show a bluer tint which would indicate ongoing star formation. The morphology suggests that this galaxy is evolving, with evidence of both older and younger stellar populations, as well as features associated with star formation within the disk. The overall structure appears relatively undisturbed, with no obvious signs of a major merger event, although minor disturbances cannot be ruled out.
