The galaxy presents as a centrally concentrated, smooth object. The light distribution suggests an elliptical morphology, with a somewhat elongated, rather than perfectly circular, appearance. It is primarily bright in the center, fading more gradually into its surrounding area. There is little to no indication of spiral arm structures or significant dust lanes, reinforcing the hypothesis that it is elliptical. The color is a mixture of blue, green, and red, hinting at a possible presence of both younger, bluer stellar populations and older, redder stars. Overall, it appears as a relatively quiescent galaxy, lacking the distinct features associated with active star formation. There may be some very subtle disturbance in the galaxy's upper regions.