The galaxy exhibits a disk-like morphology. The light distribution is dominated by a central bulge that appears mostly smooth and slightly elongated, surrounded by a less concentrated disk component. The disk shows evidence of some irregularities, potentially indicative of minor disturbances or early stages of a merger. Patches of bluer light are observed, which may be due to ongoing star formation. The galaxy displays a moderate redshift, placing it at a significant distance. Overall, the galaxy can be classified as an intermediate-type spiral galaxy undergoing some degree of interaction.
