The galaxy exhibits a generally disk-like morphology, though with some irregularity. The central region displays a bright, relatively compact core. A faint, greenish-hued halo surrounds the central core, extending further along the major axis of the disk. Evidence suggests some degree of disturbance or tidal interaction. There is a slight asymmetry in the halo's structure, which could be indicative of a minor merger event or gravitational interaction with a nearby galaxy. The redder color visible on the edge of the galaxy may be due to an abundance of older stars or dust obscuration.
