The galaxy presents as a luminous, centrally concentrated object. It appears to be generally smooth in texture, lacking prominent spiral arm structures or distinct dust lanes. The morphology suggests an elliptical or lenticular galaxy type. The central region exhibits a bright, almost unresolved core, potentially indicative of a supermassive black hole or a dense stellar population. The overall color profile appears to be relatively homogenous, with a slight shift towards bluer hues in the outer regions suggesting the potential presence of younger stellar populations. There appears to be some distortion in the symmetry of the galaxy, especially on the periphery, possibly implying past or ongoing minor gravitational interactions with another galaxy or intergalactic material. Evidence of minor disturbances such as tidal tails are not apparent.
