The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a near-elliptical morphology. The core region is significantly brighter than the outer regions, indicating a higher stellar density. The overall color appears to be slightly blue, suggesting the presence of younger stellar populations, although this could be affected by redshift. There is no apparent spiral structure or strong dust lane obscuration visible. No tidal features or other morphological disturbances are evident, suggesting that the galaxy has not experienced a major merger recently. It appears that the galaxy is generally undisturbed.
