The galaxy appears to be a spiral, seen at an angle that is neither perfectly face-on nor edge-on. There is a subtle hint of spiral arm structure, with one arm appearing more prominent. The galaxy has a somewhat diffuse and extended appearance rather than a tightly wound structure.

The central region shows a concentration of older stars, with some areas of active star formation. Overall, the galaxy exhibits a mix of stellar populations, with some regions appearing bluer, indicative of younger, hotter stars and active star formation, while others have a more reddish-yellow hue, suggesting older stellar populations. There are also some indications of irregularities in the disk, potentially due to minor gravitational interactions or internal dynamics.
