The galaxy presents as a centrally concentrated, relatively smooth object with a roughly elliptical morphology. It exhibits a radial color gradient, with a core that appears more yellow-orange, suggesting an older stellar population. The outer regions show a slightly bluer tinge, possibly indicating the presence of younger stars or ongoing star formation, though it is not highly pronounced. There is no clear evidence of spiral arms or a distinct disk structure. The overall texture appears homogeneous with no major disruptions, but there might be minor disturbances present in the form of indistinct and diffuse features. The light is generally consistent across the galaxy body and has no signs of significant ongoing mergers.
