The galaxy presents as a disk-shaped system with an inclination relative to the observer's line of sight. It exhibits a central bulge that appears relatively small in proportion to the overall disk. Hints of spiral arm structures are present, though not sharply defined. The disk shows a mottled texture suggesting regions of differing stellar density or dust obscuration.

The color profile indicates the presence of both older stellar populations, apparent towards the central bulge region, and regions of bluer light, potentially indicative of younger stars or ongoing star formation distributed throughout the disk. The apparent flattening of the galaxy suggests it could be an Sb or Sc type galaxy.