This galaxy presents an irregular morphology. The central region displays a concentrated luminosity, with a yellowish-white hue indicating a population of older stars. There is evidence of a disrupted structure, possibly indicative of an ongoing or recent interaction or merger event. The overall color suggests a mix of stellar populations, though redder components are less pronounced. Fainter extensions or tidal features are not immediately obvious, but there are some asymmetric features suggestive of disturbances.