The galaxy presents as a largely smooth, centrally concentrated object, likely an elliptical or lenticular galaxy due to its lack of apparent spiral arms or significant dust lanes. It exhibits a roughly round morphology in the image. The central region shows a brighter, more intense yellowish glow, suggesting a concentrated population of older stars. The outer regions of the galaxy appear to fade gradually into the background, with a slightly bluer hue compared to the core, hinting at the presence of a younger stellar population or some ongoing star formation, albeit at a low level. There is no obvious indication of any major merger events or tidal disturbances affecting the galaxy's overall structure, although there might be a very minor asymmetry in its outer halo. The light distribution suggests a relatively evolved system, with the majority of star formation likely having occurred in the past.
