The galaxy presents as a spiral type, with loosely wound arms emanating from a central, though not particularly prominent, bulge region. The spiral arms are quite distinct and extend outwards. The galaxy appears to be in a possible merging state with a neighbouring galaxy. This neighbour is close to the primary galaxy. There is a bridge of light between the two galaxies.

The overall colour of the galaxy is a relatively consistent blue-white, suggestive of ongoing star formation within the arms. The galaxy is oriented in a way that presents a relatively face-on view, allowing for a clear view of the spiral structure. The size of the galaxy is notable, indicating a substantial stellar population.
