The galaxy presents as a somewhat diffuse, disk-like structure with a notable central bulge. The disk shows faint spiral arm features, primarily discernible through subtle color variations. The overall color profile suggests a population of older stars, with a yellow-red hue dominating. The bulge appears smooth and concentrated, indicating a higher stellar density in this region. There appears to be some mild gravitational disturbance or interaction present in the morphology. The galaxy does not exhibit a strong blue color, suggesting a relatively low star formation rate.
