The galaxy presents a disk-like morphology, though its features are somewhat indistinct due to the image resolution. The overall color suggests a mixed stellar population, exhibiting both older, redder stars and younger, bluer stars. There's a noticeable concentration of bluer light in the central region and along certain sections of the apparent disk, hinting at ongoing star formation. The shape is more elongated than circular; it appears that it is in between a round shape and a more cigar shape. The galaxy doesn't show any obvious signs of a major merger, but there is likely minor disturbances. It exhibits an estimated physical size of approximately 6.7 kpc.
