The galaxy presents as a relatively smooth, elongated structure. There is evidence of a central bulge, with a subtle disk component extending outward. Color variations across the galaxy indicate differential stellar populations and dust distribution, the core is more red while the extremities are blue. The edges appear slightly blurred, potentially due to its distance or interactions. There is no visual indication of a major ongoing merger event, but the asymmetry could point to a minor disturbance. Overall, the galaxy appears to be in a relatively stable and evolved state.
