The galaxy exhibits a slightly irregular, disk-like morphology. The color profile suggests a mixed stellar population. The central bulge region appears yellowish, indicating the presence of older, cooler stars. The disk shows some bluer hues, especially in the outer arms, hinting at ongoing or recent star formation. Faint spiral arm structures can be discerned, though they are not sharply defined. There may be some evidence of minor tidal disturbances or interactions, as the disk appears slightly warped or asymmetric. The galaxy does not present a grand design spiral structure, appearing more flocculent overall.
