The galaxy appears to be relatively small, exhibiting a disk-like structure oriented approximately edge-on from our vantage point. The central region displays a bright, concentrated luminosity, possibly indicating the presence of an active galactic nucleus or a dense stellar population. The disk shows a gradient of colors. There is a concentration of light in the center of the galaxy, and at one end there appears to be a tidal tail. This morphology suggests a potential ongoing gravitational interaction. There is a faint glow above and below the galaxy. Overall, the galaxy exhibits a non-quiescent morphology, hinting at recent or ongoing dynamic processes.
