The observed galaxy presents as a somewhat compact object with a notable color gradient. The central region exhibits a bright, greenish-white hue, suggesting a concentration of relatively young, hot stars or active galactic nucleus activity. Surrounding this core is a more diffuse, reddish halo. The halo may consist of older stellar populations or dust. There is a slight suggestion of asymmetry in the outer halo, with a possible extension or tidal feature on one side. The overall morphology appears relatively smooth, though the faintness of the galaxy makes it difficult to discern fine details. Evidence of minor disturbances may be present in the asymmetry in the halo. Further observations with higher resolution would be required to ascertain any disk-like structure or the presence of distinct spiral arms.
