This galaxy presents as a spiral type, exhibiting a distinct, albeit somewhat ill-defined, spiral structure. The arms are not sharply delineated, appearing more flocculent in nature. The color profile suggests the presence of active star formation, evidenced by the blue hue within the spiral arms. These regions are likely sites of ongoing or recent stellar genesis. The winding of the arms is relatively tight, implying a potentially older spiral galaxy, though the blue color suggests otherwise. The galaxy displays a small central bulge, with a bar structure appearing relatively weak across the central region. Evident color gradients exist, with a generally bluer trend toward the outer edges of the disk. This suggests that the central region contains older stellar populations. There are no obvious signs of any major ongoing merging events, though there are minor disturbances within the spiral arm structures suggesting some gravitational interactions within the galaxy, and potential minor disturbances. The galaxy is oriented face-on with respect to our line of sight.
