The galaxy presents as a spiral galaxy, observed at a notable angle from edge-on. A prominent central bulge is visible, exhibiting a bright, concentrated luminosity. Fainter, less distinct spiral arms emanate from the central bulge extending outwards. These arms are patchy and irregular in structure. Blueish regions, suggestive of areas of star formation, are observed in the outer portions of the galaxy. There are also dark bands that may indicate dust lanes within the spiral structure. The overall shape appears distorted, possibly indicating an interaction with another galactic structure or other gravitational disturbances.
