The galaxy presents as a flattened, disk-like structure, although the precise inclination is difficult to ascertain due to the limitations of the image resolution. A central bulge region is apparent, displaying a smoother, more concentrated light profile compared to the outer disk. There is some evidence of defined structures, but they do not resolve clearly into spiral arms. The galaxy exhibits a color gradient, with a bluer component concentrated in the central regions, possibly indicating ongoing star formation. The outer disk appears redder in color, which might be caused by the dust reddening or the presence of older stellar populations. The overall smoothness of the light distribution suggests a potentially evolved system, possibly undergoing a transition from a more actively star-forming state. There appears to be an interacting object which may be tidally disrupted. The interaction may be the cause of some disk/halo disturbances.
