The galaxy presents as a somewhat irregular, disturbed system.  It exhibits a primarily blue hue, suggestive of ongoing or recent star formation.  There appears to be a central concentration of light, perhaps a small bulge, though it is not sharply defined.  A disk-like structure is present, but it is not well-defined and appears perturbed, with possible tidal features or disturbances indicative of an interaction or recent merger. The disk does not appear to be edge-on. Spiral arm structure is not readily apparent. There appears to be a significant amount of dust obscuring some regions, contributing to the irregular appearance.  Some reddish knots are visible within the overall blue galaxy structure, possibly representing older stellar populations or regions of dust. There is a complex morphology suggestive of significant gravitational interaction.
