The galaxy presents a flattened, elongated morphology. Its central region exhibits a bright, concentrated luminosity, appearing relatively smooth in texture, with a gradual fading of light intensity towards the outer edges. The overall color profile tends towards the bluer end of the spectrum, hinting at the presence of younger, hotter stellar populations. There appears to be a minor disturbance or slight asymmetry in the structure, perhaps indicative of past or ongoing interactions.
