The galaxy presents a generally smooth and rounded morphology. It appears as a concentrated, bright central region surrounded by a more diffuse halo. The color profile suggests a higher concentration of older stellar populations in the core, indicated by a yellowish-white hue, which transitions to a bluer tint in the outer regions, potentially indicating the presence of younger stars or ongoing star formation. There is no distinct spiral structure visible, nor any obvious signs of major disturbances or ongoing mergers, though a faint asymmetry cannot be ruled out.
