The galaxy presents as a relatively small, faint spiral, likely at a considerable distance. It is elongated in shape, exhibiting a clear disk structure. A central bulge is present, though not particularly prominent. Faint spiral arms extend from the central bulge, appearing somewhat tightly wound. The arms display a mottled texture, suggestive of regions of active star formation. The overall color is moderately blue, indicative of a moderate amount of young, hot stars, implying a ongoing, although potentially low-level, star formation rate. There is no obvious sign of a major merger event occurring, with only minor disturbances if any apparent in the morphology. The galaxy exhibits a smoothness to its overall structure.
