The galaxy presents as a flattened disk-like structure, viewed at a considerable angle. The central region exhibits a bright, concentrated luminosity profile, suggesting a prominent galactic nucleus. Extending outwards from the nucleus, the disk displays varying colors and brightness. The light emitting from the galaxy is observed to be primarily blue, indicating the presence of young, hot stars. The relative lack of strong spiral arm features and the somewhat smooth appearance of the disk suggest that this galaxy may be transitioning away from a spiral morphology or have experienced a recent disruption. There are some indications of possible tidal features on the edges of the disk, such as faint extensions or irregularities. The asymmetry in the outer regions of the disk hints at a possible gravitational interaction.
