The galaxy appears to be a spiral galaxy, viewed at an oblique angle, presenting a flattened disk-like morphology. The galaxy exhibits a central bulge region that is moderately prominent, fading into spiral arms which are easily visible. The arms display a relatively patchy distribution of light, suggesting active star formation regions. The arms appear loosely wound and can be traced outwards from the bulge. The presence of blue-ish regions indicate a population of younger, hotter stars in those arms. There is evidence of dust lanes in the galaxy. The disk shows a general inclination, which may affect the apparent shapes and magnitudes. Some irregular features and tidal disturbances may exist. Overall, the galaxy shows typical characteristics of a late-type spiral galaxy with ongoing star formation.