The galaxy presents as an elongated object with a distinct disk-like structure viewed nearly edge-on. Its overall color is yellowish-orange.

There appears to be a noticeable bulge in the central region, potentially obscuring finer details. One end of the galaxy exhibits a bluer hue. Dust lanes are suspected within the plane of the disk, contributing to the observed color variations. There may be signs of tidal disturbances or interactions.

The apparent magnitude suggests a relatively luminous galaxy. It is suspected there are signs of modest star formation activity occurring within the disk. The morphology is suggestive of a spiral galaxy undergoing some form of interaction.
