The galaxy presents as a centrally concentrated elliptical or lenticular system, appearing relatively smooth in texture, with a high degree of central luminosity. The overall shape is moderately elliptical.  The light distribution suggests an older stellar population, exhibiting a redder hue overall. There is no visually apparent spiral arm structure or significant dust lane obscuration. No signs of a major ongoing merger or tidal disturbances are visible. The observed morphology suggests a galaxy with a suppressed star formation rate, likely due to gas depletion or quenching mechanisms.
