The galaxy presents as an elliptical morphology, exhibiting a smooth, centralized concentration of light. The light distribution appears to be primarily yellow and red, potentially indicating an older stellar population. The shape of the galaxy is elongated, appearing cigar-shaped rather than perfectly round. There may be a subtle disturbance in the form of an asymmetrical halo surrounding the core. It is difficult to ascertain the precise internal structure, but the general impression is that of a mature, relatively quiescent system with no major ongoing merger events visibly disrupting its form. 
