The galaxy in question presents a complex morphology. It appears to be a disk galaxy undergoing a possible interaction or merger. The main body of the galaxy exhibits a central bulge with a yellowish hue, indicative of an older stellar population. Extending from the central bulge is a discernible disk structure that is relatively well-defined. The spiral arms appear somewhat flocculent, with regions of bluer light suggesting ongoing star formation. Faint dust lanes may be present within the disk structure. 

A secondary, smaller galaxy is positioned nearby, seemingly interacting with the larger galaxy. This smaller galaxy exhibits a more disturbed morphology, possibly due to gravitational interactions. The presence of these two galaxies suggests a close pair system. The system appears to be actively undergoing some form of interaction or merger.
