The galaxy presents a smooth, elliptical morphology. Its shape is moderately elongated, appearing more akin to a lenticular galaxy when considering its estimated redshift, albeit without a prominent disk structure visible in this image. The color appears bluish, suggesting the presence of some younger stellar populations, though it is not strongly indicative of vigorous ongoing star formation. There is no visible evidence of spiral arms, dust lanes, or other distinct features. There is no apparent tidal debris or morphological distortions to suggest recent major mergers or interactions. There is only a slight chance of a minor merger disturbance based on the image. The light appears to be concentrated centrally, indicating a higher density of stars towards the core. There is a gradual decrease in the surface brightness from the core outwards.
