The galaxy presents a spiral morphology, exhibiting a distinct disk structure. Two prominent spiral arms are clearly visible, extending from a central bulge. The arms appear to be moderately wound. The central bulge seems to be of a moderate size. The presence of a bar-like structure traversing the central region cannot be definitively confirmed from visual inspection alone, however there does appear to be a slight elongation across the bulge. Evidence of recent or ongoing star formation is suggested by the bluer colors visible along the spiral arms. A potential minor disturbance or interaction is suggested in the visual, possibly indicating an early stage merger, based on a secondary less defined object appearing to be connected via a slight bridge of material.
