The galaxy presents as a moderately faint, bluish, disk-shaped object. The blueness suggests ongoing star formation. There is potential evidence of a disturbance or merging event, indicated by an irregular shape and hints of disrupted structure. The disk appears to have a central concentration, potentially a bulge, although this is not sharply defined. The galaxy does not display a pronounced spiral arm structure but exhibits a somewhat chaotic appearance, supporting the possible merger scenario. Its apparent small size and faintness indicate it is likely a low-mass system.
