The galaxy presents as a relatively smooth, disk-like structure with a moderate degree of central concentration. The core region exhibits a yellowish-orange hue, suggesting an older stellar population, while the outer disk appears bluer, potentially indicating more recent star formation. The galaxy displays a slight elongation, leaning toward a cigar-shaped morphology. There is a subtle hint of minor disturbance in the outer regions of the disk, although no major merging event is immediately apparent.
