The galaxy presents as a spiral structure with a prominent bulge. The spiral arms appear tightly wound, extending from the central bulge. There is a strong indication of a tidal tail or distorted morphology suggesting a possible interaction or merger event. The bulge exhibits a yellowish hue, indicative of an older stellar population. The spiral arms show bluer regions, potentially indicating areas of active star formation. The overall color suggests a galaxy undergoing significant star formation with the presence of both young, blue stars and an older, redder population in the central bulge. There seems to be a distinct, separate component nearby that may have been involved in the interaction with the galaxy.
