The galaxy presents as a moderately luminous object with a generally smooth morphology. The central region exhibits a pronounced concentration of light, appearing yellowish, suggesting a population of older stars.  Moving outwards from the core, the surrounding region is less concentrated and takes on a bluer hue, indicative of younger stellar populations or ongoing star formation. The overall shape of the galaxy is somewhat elliptical, lacking a strong spiral structure or a distinct disk. There may be some minor asymmetry or irregularity present in the outer regions, potentially suggesting past interaction or disturbance, but this is difficult to definitively ascertain given the resolution. No pronounced tidal tails or other clear signs of a major ongoing merger are evident. The galaxy's light is redshifted, placing it at a significant cosmological distance.
