This galaxy appears to be a relatively small, disk-shaped system with a moderate degree of internal structure. The light distribution suggests a central bulge, though it is not particularly prominent. There's evidence of a disk component, hinted at by a slight elongation, though the disk structure is not well-defined; it seems somewhat disrupted. The color suggests the presence of ongoing star formation. There is a noticeable disturbance to the overall shape and light distribution, possibly indicating an interaction or merger event. There also may be some tidal features.
