This galaxy exhibits a disk-like morphology, viewed at an oblique angle. There is evidence of spiral arm structure, although the arms themselves appear somewhat fragmented and lack clear definition. The central bulge region is moderately prominent and possesses a bright, concentrated core. A faint, elongated structure extends from the main body of the galaxy; it is unclear if this is a tidal tail or a feature within the galactic disk. The galaxy displays a color gradient, with the core and bulge exhibiting a bluer hue, while the outer regions and arm structures appear redder in color, which could indicate variations in stellar populations or dust content. There is potential for interaction or merger with another galaxy.
