The galaxy appears as a relatively smooth, disk-shaped structure with a slight inclination to our line of sight. It exhibits a central bulge that is brighter and more concentrated than the surrounding disk. There may be some hint of spiral arm structure, though it is not very pronounced or well-defined in this image. The overall color suggests a mix of stellar populations, with the central region appearing slightly redder. There may be a minor disturbance, but the galaxy mostly looks unperturbed, though the data suggest it might be the early stages of merging with a small companion.

