The galaxy presents a diffuse, somewhat amorphous morphology. Its overall shape is not well-defined; it appears elongated with a faint halo extending beyond a brighter central region. There is no clear evidence of spiral arms or a distinct disk structure. The light distribution within the galaxy is uneven, suggesting potential irregularities or disturbances within its structure. A bluer component is apparent around the edges, possibly indicating recent star formation activity in these regions. The redder core may be indicative of an older, more evolved stellar population. Further observations and spectral analysis would be required to fully characterize its composition and evolutionary state. There is possibly a minor interaction or disturbance visible based on the asymmetry.
