This galaxy appears to exhibit a flattened, disk-like morphology when viewed at its current orientation. The central region is dominated by a bright, concentrated core, indicative of a possible bulge component. Fainter emissions suggest a structure extending outwards from the central bulge. A notable distortion is observed in what would be the spiral arm structure on either side of the galaxy; they are not clearly defined and appear diffuse. Some asymmetrical features suggest the possibility of a gravitational interaction with another celestial body. The observed color indices imply that the inner regions are bluer, and the outer emissions are more red, indicating a likely difference in stellar populations, with younger stars at the center and older stars farther out. Overall, the galaxy is a peculiar object, with a relatively featureless disk coupled with signs of disturbance in the surrounding regions.
