The galaxy presents as a spiral type, exhibiting clear arm structures extending from a central bulge. These arms appear somewhat flocculent, with regions of enhanced brightness that suggest active star formation. The bulge appears prominent, with no dust lanes easily visible. Overall, the galaxy's light distribution seems smooth, indicating a more evolved system. The galaxy is inclined relative to our line of sight, with the angle of inclination causing a slight visual asymmetry. There are also some signs of disturbance, or faint distortions in the shape of the galaxy, that could indicate possible mergers or interactions.
