The galaxy presents a morphology characterized by both smooth and featured elements. It exhibits a central bulge region with a yellowish hue, suggesting a population of older stars. Emanating from this central region is a faint, diffuse disk structure.

There are indications of possible gravitational interaction or disturbance. The outer regions of the disk exhibit slight asymmetries, and there is a hint of a tidal tail or bridge-like structure extending from the main body of the galaxy. This could be due to a recent or ongoing minor merger event. The galaxy does not appear to be undergoing a major merging event. 

The overall color profile indicates active star formation within the disk, although to a lesser degree than one might expect from a spiral galaxy. There are some indications of dust lanes or patches of obscuration. Further analysis with higher resolution images and spectroscopy will be needed to confirm the dynamics of the galaxy.
