The observed galaxy presents a clear spiral structure, exhibiting prominent and loosely wound arms emanating from a central bulge. The arms display variations in color, indicating regions of differing stellar populations and dust content. Evidence suggests ongoing star formation within the spiral arms, particularly in localized areas exhibiting a bluer hue. A bar-like feature may be present traversing the central bulge, but its definition is weak. The galaxy's disk appears to be viewed at a slight angle, deviating from a perfect face-on orientation. The central bulge appears moderate in size compared to the overall galactic disk. Some morphological irregularities and light distortions hints that this galaxy may be undergoing or have recently undergone a minor or major merger.
