The galaxy presents a disturbed morphology, potentially indicative of a recent or ongoing merger event. Its overall shape is irregular, lacking a well-defined spiral or elliptical structure. A dominant feature is an elongated, diffuse component with a brighter central concentration. The light distribution is uneven, with areas of enhanced brightness and patchy regions. These brighter regions likely correspond to areas of active star formation within the galaxy. The galaxy exhibits a blueish color, suggesting a relatively young stellar population. This blue color contrasts with the galaxy's red shift, which could mean that the dust is causing it to appear more red than it actually is.
