The galaxy presents a largely smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity, transitioning into a slightly irregular halo structure. There is evidence of bluer light distribution, suggesting the presence of younger stellar populations within the galaxy's composition. A distinct, relatively small region of intense, localized emission, potentially indicative of active star formation, is observable near the galaxy's periphery. Overall, the galaxy exhibits a dominant spheroid component, and the light appears to be relatively concentrated. There is a noticeable lack of spiral arms or a well-defined disk structure. There may be some subtle disturbances or faint features in the outer regions, but they are not prominent enough to classify this as a major merger event.
