The galaxy presents as a somewhat elongated, smooth structure. There's a subtle color gradient, with the central region appearing slightly bluer than the outer edges, possibly indicating a higher concentration of younger stars in the core. The galaxy does not exhibit prominent spiral arms or a well-defined disk. Its overall shape is neither perfectly spherical nor highly flattened, suggesting an intermediate elliptical morphology. There appears to be a minor disturbance or asymmetry in the galaxy's light distribution on one side, which might suggest a past or ongoing interaction with a smaller companion. There is no evidence of a major ongoing merger, but the asymmetry could potentially evolve into a more substantial interaction in the future.
