The galaxy presents a moderately bright, diffuse appearance. Its central region is dominated by a concentrated, luminous core. The light gradually decreases from the center outwards, suggesting a centrally concentrated mass distribution. The galaxy appears generally smooth in structure with a faint disk. There is a low probability of a major merger and low probability of minor disturbance. The galaxy is slightly elongated, with a non-negligible probability of an artifact present in this image. The color profile is predominantly white with faint blue or green in some regions. 
