The galaxy appears to be a relatively compact system, exhibiting a smooth overall structure with a hint of a disk-like morphology. The central region displays a brighter, concentrated luminosity. There is some distortion of the main body, with noticeable asymmetry suggesting potential minor gravitational interactions. Color gradients are subtle; the central region shows a redder hue, indicative of an older stellar population, while the outer regions display bluer tones possibly associated with younger star formation.
