The galaxy presents an elongated morphology. It appears to be undergoing some form of interaction or disturbance, as evidenced by the asymmetry and the faint, plume-like extension emanating from the main body. The central region appears brighter and more concentrated, potentially indicative of a bulge component. The overall color is relatively red, suggesting a population of older stars and/or significant dust obscuration, though there is a hint of bluer colors in the plume suggesting possible star formation. Based on the smooth appearance it may be an elliptical galaxy, but there is also evidence that indicates it might be a merging galaxy. Further investigation is required to determine it's true identity.
