The galaxy presents as a centrally concentrated object with a roughly circular morphology, although the pixelated nature of the image limits a precise determination of its shape. There appears to be a luminous core, likely indicating a substantial concentration of stars and potentially an active galactic nucleus. The galaxy exhibits a blueish hue in the center. Some slight extensions or irregularities in the outer regions of the galaxy are apparent, potentially hinting at minor tidal disturbances or interactions with smaller companion galaxies. However, based on this image alone, it is difficult to ascertain the precise nature of these features. The overall appearance suggests a relatively compact galaxy at a considerable distance. Higher resolution imagery and spectroscopic data would be necessary to confirm the presence of any merger activity and to characterize the galaxy's stellar populations and dynamics further.
