The galaxy presents a prominent disk structure, viewed at an angle that suggests a significant inclination relative to our line of sight. Spiral arms are visible, exhibiting a somewhat patchy and flocculent morphology. These arms appear moderately tightly wound.

A central bulge is discernible, contributing noticeably to the overall brightness profile of the galaxy. The bulge seems to be of moderate size relative to the overall disk.

There is evidence of potential interaction or recent merger activity. The outer regions of the disk show a slightly disturbed morphology, possibly indicating tidal interactions.

The galaxy displays a color gradient, with the central bulge exhibiting a more yellow/red hue, suggestive of an older stellar population, while the spiral arms are bluer, potentially indicating ongoing star formation.

Overall, the galaxy presents characteristics consistent with a spiral galaxy undergoing, or having recently undergone, some form of gravitational interaction. The presence of spiral arms and color variations indicates active regions of star formation within the disk.
