The galaxy presents as a disk-shaped system, viewed at a significant inclination. A pronounced central bulge is observed, exhibiting a smooth, concentrated distribution of light, appearing yellowish-white in color. The disk component displays a bluer hue, suggesting the presence of ongoing star formation. The overall form of the galaxy is elongated, with a length that appears to be several times greater than its width. One edge appears truncated, or there is an object in the foreground. The galaxy exhibits a moderate degree of internal structure, possibly indicating spiral arm segments. The light distribution transitions smoothly from the bulge to the disk, with no distinct breaks or rings visible. There appears to be a tail like structure protruding from one side of the galaxy. 
