The galaxy presents as a relatively compact, face-on object. The central region exhibits a bright, concentrated luminosity profile suggesting a prominent galactic nucleus or core. The light emission extends outwards from this central point in a diffuse and somewhat irregular manner, indicating a complex structure. There is an apparent asymmetry to the galaxy's overall shape, with extensions or plumes of less intense light visible on either side of the brighter core. One area seems to have a slight reddish hue, indicating the presence of potentially older stars or dust. The morphology of the galaxy suggests possible interactions or disturbances, but there is no conclusive evidence for major mergers. 
