The galaxy presents as a disturbed system, possibly undergoing a merger event. There is a distinct, bright central bulge with an elliptical morphology. This central region exhibits a yellowish hue, suggesting an older stellar population. Extending from the central region, fainter structures or tails are observed, indicative of gravitational interaction. The presence of blueish regions suggests the presence of younger star formation. Overall, the galaxy's morphology is irregular and complex.
