The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. Its overall shape is approximately round, displaying minimal deviation from circular symmetry. There is a subtle colour gradient, transitioning from a yellowish hue at the core to a slightly redder colour in the outer regions. This colour shift might indicate varying stellar populations or dust content across the galactic structure. There is no discernable spiral structure or bar feature. No significant tidal disturbances or signs of ongoing mergers are apparent from visual inspection. The galaxy appears relatively undisturbed.
