The galaxy presents as a somewhat elongated, although mostly smooth, structure. There is evidence of a disk-like morphology, but no clear spiral arm structure is visible in this image. The color gradient suggests the presence of both older stellar populations, implied by the redder hues, and regions with more recent star formation indicated by the bluer colors in a few knots of brightness. The main body appears relatively undisturbed, suggesting no recent major merger events, although a minor disturbance or interaction could be plausible given the slight asymmetry and the possible tidal feature/tail-like structure. The galaxy's overall shape leans towards being cigar-shaped rather than perfectly round. Based on the color profile, the galaxy appears to be of intermediate mass. The faintness of the galaxy suggests it is at a considerable distance, evidenced by the measured redshift. Overall, it appears to be a disk galaxy that may have some past interactions.
