The galaxy appears to be a relatively smooth, centrally concentrated system. Its morphology suggests an elliptical or lenticular type, with a high degree of symmetry and no discernible spiral arm structure. The color profile indicates a dominant yellowish hue in the central region, possibly indicative of an older stellar population. The outer regions are fainter and slightly bluer, which could suggest the presence of some younger stars but this is likely minimal. There are no signs of major disturbances or interactions. It appears to be a fairly evolved and undisturbed galaxy. Based on the apparent roundness, it is unlikely to be an edge-on disk galaxy.
