The galaxy presents a generally smooth morphology, although there appears to be some disturbance present. It exhibits an overall disk-like shape, transitioning from a rounded central region outwards. The color profile suggests recent or ongoing star formation, indicated by the blue hue, particularly concentrated in what appears to be spiral arm structures or regions within the disk. A significant portion of the galaxy's light emanates from a relatively compact central region, likely the galactic bulge or nucleus. There is an indication of an interacting or merging system.
