The galaxy presents as an elliptical morphology, characterized by a smooth, largely featureless appearance, exhibiting a high degree of central concentration. The light profile transitions smoothly from the core outwards. The galaxy appears elongated, with its major axis significantly larger than its minor axis. It exhibits a color gradient, transitioning from a yellowish-red core to a bluer outer halo. The core likely contains an older stellar population, while the bluer halo may be evidence of younger stars or recent minor disturbances. No prominent dust lanes or spiral arm structures are discernible. There is evidence of a possible minor disturbance in the morphology, potentially indicating a recent or ongoing merger event. Based on the light from the galaxy, it exhibits a relatively high mass and moderate star formation rate, indicative of an intermediate stage in its evolution.
