The galaxy presents a moderately luminous appearance, exhibiting a discernible disk-like morphology that is neither perfectly circular nor highly elongated. The primary body of the galaxy displays a smooth texture, indicating a relatively homogenous stellar population. However, there are subtle, localized irregularities that may suggest minor disturbances or interactions. The galaxy's color profile transitions across its structure, revealing variations in stellar populations. The brighter region suggests a more substantial population of young, hot stars, whereas the orange region suggest a substantial population of older stars.
