The galaxy presents as a diffuse, somewhat irregular object. It has a significantly brighter central region, suggesting a concentration of stars or an active galactic nucleus. The galaxy appears elongated, hinting at a disk-like structure, although no spiral arms are readily apparent. There might be some degree of minor disturbance in the galaxy's morphology. Faint tidal features or disrupted structures can be observed, indicating recent or ongoing gravitational interaction with another galaxy. 

The galaxy displays a color gradient, with the core appearing slightly bluer than the outer regions. This might suggest the presence of younger, hotter stars in the core, or dust reddening in the outer regions. Overall, the image indicates a galaxy of moderate size and luminosity, potentially undergoing some degree of interaction or internal disturbance.
