The galaxy appears as a centrally concentrated object with a relatively smooth overall morphology. There is a slight elongation, but it is generally round in appearance. The galaxy exhibits a bright central region that fades into a more diffuse halo. The color profile suggests a population of older stars with a likely significant red component. There is a hint of a blueish hue on the edges, suggesting the presence of some younger, star-forming regions. There are no obvious spiral arms or a distinct disk structure visible. Based on its morphology, the galaxy may be an elliptical or lenticular galaxy. There is some evidence of minor disturbance in the galaxy's shape, potentially indicating an ongoing or past merger event.
