The galaxy exhibits a disk-like morphology, although it is not sharply defined. There are regions of varying intensity that suggest some features or spiral arm structures are present. The galaxy displays a color gradient, with some areas appearing more reddish compared to others that are slightly more bluish. This may be due to differences in stellar populations or dust content. The general appearance of the galaxy suggests it is likely undergoing some minor interaction or disturbance, but not a major merger. There is no obvious, large-scale distortion of the disk.
