This galaxy presents as a somewhat elongated, disk-like structure viewed nearly edge-on. The central bulge appears indistinct, with a relatively uniform brightness distribution across the main body of the galaxy. There is subtle bluing present, concentrated primarily within the disk, suggesting the presence of younger stellar populations and ongoing star formation activity, albeit possibly at a low rate. Faint tidal features are suspected near the edge on the western side, potentially indicative of a minor interaction or disturbance. Overall, the galaxy exhibits a smooth morphology, however it cannot be said for certain whether the source is a disk galaxy or elliptical galaxy with a disk-like shape.
