The galaxy presents a largely smooth and centrally concentrated morphology. The light distribution appears to be dominated by an elliptical, spheroidal component with a high degree of radial symmetry. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy exhibits a color gradient, transitioning from a more yellow-white hue in the central region to a slightly greener color in the outer regions. There appears to be a subtle, low-surface brightness halo extending beyond the main body of the galaxy. Overall, the galaxy presents a relaxed appearance with no signs of ongoing major mergers or significant tidal disturbances, although a subtle disturbance cannot be ruled out.
