The galaxy appears as an elliptical or lenticular type, exhibiting a relatively smooth and concentrated light distribution. It demonstrates an elliptical morphology with a high degree of central concentration, indicating an older stellar population. There is no apparent spiral arm structure or active star formation regions that are visibly clear from the data. The colour of the galaxy appears redder, suggesting it is likely a more evolved system, which is consistent with elliptical morphologies. Overall, the galaxy appears as a relatively massive system, given its apparent size and luminosity. There are indications of some minor disturbances or tidal features, but the overall morphology seems relatively undisturbed with most votes indicating this galaxy is not undergoing a major merger.
