The galaxy presents as a flattened elliptical morphology with a central bulge. The core region exhibits a concentrated, bright golden hue, potentially indicative of a dense population of older stars. Surrounding the core, the luminosity gradually decreases, transitioning into a diffuse halo. Within the halo, traces of bluish components can be distinguished, suggesting some presence of younger, hotter stars or star-forming regions. The galaxy's overall shape is relatively smooth, with no obvious spiral arms or significant tidal features, indicating a dynamically settled structure. There is little evidence of active galactic nuclei activity in the form of relativistic jets, or extreme fluxes of radiation.
