The galaxy presents as a distorted spiral, exhibiting significant morphological disturbance suggestive of an ongoing or recent merger event. The central bulge appears relatively bright and large, with a moderate contribution to the overall galactic luminosity. There are some signs of a bar structure present, but it is not particularly prominent. Evidence of spiral arm structure is visible, however, these arms are irregular and asymmetric, indicating gravitational interaction. A tidal tail extends from the main body of the galaxy, a further indication of a merger event. The galaxy's color is predominantly blue, suggesting a presence of younger stars and active star formation. There are indications of possible dust lanes visible within the spiral arms. Overall, this galaxy appears to be an actively evolving system, currently undergoing a dynamic interaction with another galaxy.
