The galaxy presents as a spiral, oriented at an oblique angle relative to the observer. A prominent central bulge dominates the core, exhibiting a yellowish-white hue, suggesting an older stellar population. Fainter spiral arms extend outwards, displaying hints of blueish regions possibly indicating areas of active star formation. Two distinct spiral arms are clearly visible with medium winding, tracing outwards from the central bulge. The arms are not perfectly symmetrical, showing some irregularities. The presence of a bar feature is visible in the center of the galaxy. No signs of major interactions or mergers are readily apparent, although there may be some minor tidal disturbance.
