The galaxy exhibits a roughly circular morphology, with a bright, concentrated central bulge. The overall color is dominated by a blue-green hue, suggestive of recent or ongoing star formation activity. 

There is evidence of spiral arm structure, though it appears somewhat disrupted and patchy. The arms display variations in color, with some regions appearing more red, potentially indicating older stellar populations or dust obscuration. 

The outer regions of the galaxy appear more diffuse and less structured. There is some indication of tidal features or faint streams extending from the main body, possibly hinting at a past or ongoing interaction with another galaxy. The overall structure suggests possible disturbance with mild distortion of the galaxy's disk.
