The galaxy presents a somewhat elongated, disk-like morphology, though with a significant bulge component. The central region exhibits a high concentration of light, appearing yellowish, indicative of an older stellar population. Surrounding this core, we observe a slightly bluer and more diffuse disk component, suggesting the presence of younger stars and possibly ongoing star formation.

There appears to be some asymmetry in the disk, perhaps hinting at minor tidal interactions or internal disturbances. No well-defined spiral arms are readily apparent. Overall, the galaxy appears to be transitioning between a relatively smooth morphology and one displaying more prominent disk features.
