The galaxy presents a complex morphology, likely indicative of an ongoing or recent merger event. Its structure is noticeably disturbed, lacking a well-defined spiral or elliptical shape. Patches of diffuse blue light are present, suggesting regions of active star formation. The overall color appears relatively blue, leaning towards younger stellar populations. Indications of tidal tails or bridges are visible, implying gravitational interaction with another galaxy in the past or present. There is no obvious central bulge. The galaxy has an estimated effective radius of 3 kiloparsecs, but its irregular shape makes this measurement uncertain. 
