The galaxy presents as a somewhat elliptical, disk-like structure with a noticeable bulge. The color gradient suggests an older stellar population.

A distinct, irregular region is visible at one end, exhibiting a clumpy morphology. The color in this region skews redder and more orange than the disk itself, suggestive of ongoing or recent star formation.

Overall, the galaxy appears relatively smooth and well-defined, although the irregular region implies some level of disturbance. The smoothness of the main body is also a sign of low star formation activity.
