The galaxy presents as a relatively compact, elliptical-like structure. Its overall shape is smooth and rounded, with a high degree of central concentration. There is a distinct lack of any spiral arm features or obvious disk component. The light profile appears to decline smoothly from the center outwards. Color gradients are subtle, but the core seems slightly more red-shifted compared to the outer regions, potentially indicating an older stellar population concentrated towards the center. There are no obvious signs of recent major merger events or significant tidal disturbances, although a very faint asymmetry cannot be entirely ruled out. The galaxy appears to be relatively isolated.
