The galaxy presents a flattened, disk-like morphology. It appears to be a spiral galaxy viewed at a relatively high inclination, possibly close to edge-on. Evidence of spiral arms is subtle but suggested by irregular light distribution across the disk. A central bulge is apparent, moderate in size and luminosity compared to the overall galactic disk. There is a suggestion of a bar-like structure in the central region.

The color profile indicates a higher concentration of older stellar populations toward the bulge, exhibiting a yellowish-red hue, while bluer regions are distributed along the disk, possibly tracing areas of recent star formation. The galaxy appears to be experiencing minor disturbances, perhaps an early stage interaction with a smaller companion galaxy. Overall, the object appears to be a late-type spiral galaxy with moderate ongoing star formation.
