The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light distribution that gradually fades towards its periphery. The central region displays a yellow-white hue, indicating a population of older stars. This color shifts subtly to a bluer tone towards the outer edges, possibly suggesting the presence of some younger stellar populations, or low-level star formation. The galaxy's overall shape is elongated, with a major axis to minor axis ratio of approximately 3:2, hinting at a deviation from a perfectly spherical form. There is no apparent spiral structure or dust lane features visible in this image.
