The galaxy presents an elongated, disk-like morphology, viewed nearly edge-on from our vantage point. A central bulge is discernible, appearing a warmer, more yellowish hue. The disk itself exhibits a bluer tint, suggesting the presence of younger stellar populations and ongoing star formation. There are hints of some disturbances to the disk structure, possibly indicating tidal interactions or recent minor merger events. A fainter, adjacent object nearby seems to be interacting with the main galaxy. The galaxy is a very luminous object, and hosts a moderate amount of star formation. The galaxy appears large in size.
