The galaxy presents as a disk-shaped object, oriented at an angle relative to our line of sight. It exhibits a moderate degree of internal structure. A central bulge region is apparent, with a yellowish-orange hue, possibly indicating an older stellar population. Extending outwards from this central region, a disk structure is visible.

One side of the disk appears to be more disrupted, with clumpy, reddish areas that could potentially be indicators of active star formation regions or dust lanes. The other side of the disk appears relatively smoother and more uniform, fading into the background sky.

Overall, the galaxy appears to be in a stage of moderate evolution, possibly undergoing minor interactions.
