The galaxy presents a generally smooth appearance, with a near-spherical morphology. There appears to be no distinct spiral arm structure or a prominent bar. The galaxy appears to be a diffuse, centrally concentrated object, with a smooth falloff in luminosity from the core. Subtle color variations are present, with a bluer central region and a progressively redder halo. These color variations suggest differing stellar populations, with younger, bluer stars concentrated towards the center and older, redder stars dominating the outer regions. There is a low level of noticeable disturbance in the system, although there may be a very faint tidal tail stretching out from the galaxy. This disturbance is subtle but is consistent with a past or ongoing minor merger event, although this is tentative. Overall, the galaxy appears to be of intermediate luminosity and mass. Given the redshift, its light has been stretched due to the expansion of the universe.
