The galaxy presents as a spiral with two distinct arms that extend far from the central bulge. The arms are loosely wound and exhibit a blue hue, suggesting active star formation. The central bulge appears yellow-white, indicating an older stellar population. The galaxy is inclined relative to our line of sight, offering a view of its disk-like structure. A subtle bar-like structure appears to bisect the bulge, and a faint dust lane appears along the near arm. Evidence of some gravitational disturbance or minor merger event may be present as irregularities in the outer structure, as the one tidal stream extends farther away than the other.
