The galaxy presents as an elliptical or lenticular type system, exhibiting a smooth, diffuse light profile. Its shape is moderately elongated, appearing somewhat like a flattened spheroid. The central bulge is prominent and has a concentrated appearance. The color gradient transitions smoothly from a redder core to a slightly bluer outer halo. There is no discernible evidence of spiral arm structure, or ongoing major mergers. Subtle asymmetry might indicate a minor interaction or internal disturbance. The system appears relatively isolated.
