The galaxy presents as a slightly elongated structure, potentially cigar-shaped. The light distribution suggests a central bulge that dominates the galaxy's overall brightness. The color of the central region appears more yellow, possibly indicating an older stellar population within the bulge.

A fainter, bluish region is observed on one side of the main galactic body, suggesting a region of active star formation. The overall morphology leans towards a system undergoing some form of gravitational interaction or disturbance, although a major merger is not immediately apparent. This is based on a slight distortion to the edges of the galaxy, and the separated blue region.
