This galaxy exhibits a morphology that is predominantly smooth, although there are some subtle features present. The central region displays a bright, concentrated core, indicative of either a dense stellar population or active galactic nucleus. Surrounding the core, there's a diffuse, almost amorphous halo, which could be a spheroidal component. Faint extensions or tidal features hint at possible gravitational interaction with a nearby companion, or a past merger event. The galaxy displays a color gradient, with the core appearing bluer than the outer regions. This color difference may suggest a younger stellar population dominating the core, while older, redder stars populate the halo. Overall, the galaxy presents as a relatively compact, elliptical-like system with subtle signs of past or ongoing interactions.
