The galaxy presents as a single, relatively compact object. It exhibits a smooth, elliptical morphology with a high degree of central concentration. The color appears generally white, suggesting a mixture of stellar populations but possibly dominated by older, less massive stars. There's a subtle indication of a faint, diffuse halo surrounding the central region. No distinct spiral arms or bar structures are discernible. The overall appearance suggests a galaxy that has undergone significant evolutionary processing, potentially exhibiting a relatively low ongoing star formation rate. There is no evidence of any major ongoing merger events or tidal disruptions.