The galaxy appears as a relatively compact object with a partially smooth structure. There is evidence of a disk-like morphology. The object presents as an intermediate shape between a perfect circle and an elongated form. There are indications of disturbances to the galaxy's structure, implying minor interaction or possible merging event. The light distribution suggests the presence of both older stellar populations and ongoing star formation. The galaxy's colour profile indicates moderate star formation activity. Overall, the galaxy is a relatively luminous system with a significant stellar mass.
