The galaxy presents as a single, relatively compact object. Its overall morphology appears largely smooth with a centrally concentrated bulge. Evidence of a disk structure is weak. Color gradients indicate a bluer core, potentially indicating recent star formation, surrounded by a somewhat redder halo. Slight asymmetries may suggest possible tidal disturbances or minor interactions with nearby galaxies. The overall structure is mostly undisturbed, lacking clear evidence of major mergers or significant distortions.
