The galaxy presents as a disk-shaped system, viewed at a significant inclination. A central bulge is apparent, exhibiting a yellowish hue. This color suggests a population of older, cooler stars concentrated in the galactic center. The disk component appears bluer in the outer regions, indicative of ongoing star formation and a population of younger, hotter stars. The disk shows some irregularity. It lacks a clearly defined spiral structure and is suggestive of a flocculent or somewhat disordered morphology. There is no clear evidence of a major ongoing merger, although some minor disturbances might be present. The overall appearance suggests a galaxy with a moderate mass and a relatively low specific star formation rate.
