The galaxy exhibits a disturbed morphology, appearing to be undergoing a potential merger event. Two distinct components are discernible, one presenting a bluer hue and a diffuse structure, possibly indicative of active star formation. The second component displays a yellower-orange color, potentially due to an older stellar population or dust obscuration. A tail like structure or tidal arm can be observed possibly due to a gravitational interaction, suggesting ongoing tidal forces at work. The overall shape is elongated and asymmetrical. The galaxy is likely experiencing significant disruption to its structure. There are very little dust lanes visible. It is a faint object.
