The observed galaxy presents as a disturbed system. Its morphology deviates significantly from a regular elliptical or spiral structure. The majority of the galaxy appears smooth, yet irregular. One tidal tail is clearly visible, which is located on the lower left side of the galaxy. The visible light distribution indicates ongoing or recent gravitational interactions. There is a slight blueish tint in some areas of the galaxy, but not enough to describe it as a star forming region. The color profile ranges from red and orange near the center, and then a dark violet throughout the rest of the galaxy. This may suggest a change in stellar populations, dust composition, or redshift effects across the galaxy's structure. 
