The object presents as a moderately sized galaxy, approximately circular in overall appearance. The light distribution appears patchy and irregular, with faint, diffuse regions indicative of ongoing star formation. There is no distinct central bulge evident, suggesting a disk-dominated morphology or a galaxy undergoing significant disruption. The color gradient across the galaxy is subtle, with a generally blueish-green hue, and there is a slight possibility of a faint tidal tail or asymmetric feature hinting at gravitational interaction with another galaxy. However, this feature is difficult to distinguish from background noise and artifacts. There is potential evidence of some level of disturbance within the galaxy's structure, but it is not definitive. 
