The galaxy appears as a relatively compact object. It has a central bright region suggesting a concentrated nucleus or bulge. A fainter, more diffuse structure extends outwards, possibly indicating a disk or halo component. There are hints of asymmetry in the outer regions, with one side appearing more extended or disturbed than the other. The color distribution is not uniform, with the central region exhibiting a bluer hue compared to the more reddish outer parts. This color variation could imply differences in stellar populations or dust content within the galaxy. There is a faint "plume" like structure extending downwards. Overall, the galaxy's morphology suggests it may be undergoing or have undergone some form of interaction or disturbance.
