The galaxy presents a disturbed morphology, indicative of an ongoing or recent interaction. The main body of the galaxy appears diffuse, lacking a clearly defined spiral structure or elliptical shape.  A noticeable tidal tail or plume extends from the galaxy's central region, suggesting gravitational disruption.

There is an indication of active star formation within certain regions of the galaxy, particularly within the disturbed areas. Color gradients suggest a mix of stellar populations. Based on the redder color towards the center, there may be an older stellar population, or increased dust obscuration. The overall low surface brightness makes detailed morphological classification challenging. The irregularity and disturbed features of the galaxy suggest an interaction or merger event is influencing its current form and stellar populations. Further investigation via spectroscopy and higher-resolution imaging would be beneficial to determine the exact nature and stage of the interaction, and to characterize the star formation history of the galaxy.
