The galaxy appears as a centrally concentrated, diffuse object with a generally smooth morphology. It exhibits a rounded shape, displaying minimal disk-like features or pronounced spiral arms. There is a slight color gradient from the center towards the outer regions, with the core exhibiting a slightly brighter, whiter hue, potentially indicating a higher concentration of older stars and/or a dustier interstellar medium. The outer regions appear fainter with hints of a bluer tint, which could be due to patches of younger stellar populations. There is no clear indication of ongoing merging activity or significant tidal disturbances in the image, although subtle asymmetries may be present in the brightness distribution. Overall, the galaxy appears relatively undisturbed with a likely redshift indicating a significant distance.
