The galaxy presents as a moderately bright, elliptical or lenticular system with a smooth, featureless appearance. The core of the galaxy exhibits a concentrated luminosity, suggesting an older stellar population likely dominated by yellow and red giants. Moving outward from the center, the light becomes more diffuse. There appears to be a faint blue or green tint along one edge of the disk, possibly indicating regions of more recent, albeit subdued, star formation. The galaxy's shape tends toward an elliptical form, with a slight elongation. There is no evidence of prominent spiral arms, bars, or significant tidal disturbances, indicating a relatively quiescent, non-merging state. The galaxy is at an intermediate redshift, suggesting it is at a considerable cosmological distance.
