The galaxy presents as an elliptical morphology with a smooth light distribution, exhibiting a relatively high degree of central concentration. Its color profile appears generally redder toward the core, transitioning to a slightly bluer hue in the outer regions. There is no prominent evidence of distinct spiral arms or a well-defined disk structure. Subtle irregularities in the outer envelope suggest the possibility of minor tidal disturbances or recent accretion events, though a definitive merger classification is challenging based on the available imagery.
