The galaxy presents as a spiral type, observed at a moderate inclination. Spiral arms are distinctly visible, originating from the central bulge region and extending outwards. The arms appear relatively well-defined, exhibiting a clumpy structure indicative of ongoing star formation regions. The central bulge has a moderate size, emitting a yellowish color, suggesting an older stellar population. There may be a bar-like feature across the central region of the galaxy. The overall structure doesn't show signs of major interaction or merging events, but could show slight disturbances. There is a disk present as well, which may be close to edge on. There are no other large nearby companions.
