The galaxy presents as a relatively smooth, elongated structure. It exhibits a noticeable color gradient, transitioning from a yellowish core to a redder periphery. The central region appears brighter and more concentrated, suggesting a higher density of stars and potentially an older stellar population. The overall shape is indicative of a disk-like structure viewed at an oblique angle. There may be some minor gravitational disturbances present within the galaxy. A secondary, smaller structure is observed near the main galactic body, possibly indicating an interacting companion or a tidal feature. There appears to be a low rate of star formation.
