The galaxy presents as a singular, largely featureless object, displaying a smooth, elliptical morphology. The light profile appears centrally concentrated, exhibiting a radial gradient that gradually diminishes from the core outwards. The central region displays a yellow hue, suggesting a population of older stars. There is a noticeable lack of blue light, which could indicate a low rate of ongoing star formation within the observed bands. No prominent spiral arms, dust lanes, or other significant morphological features are discernible. The overall impression is that of a mature, quiescent galaxy with a significant spheroidal component. Subtle disturbances may be present, but are not easily discernible in this image.
