The galaxy presents as an elliptical morphology, appearing largely smooth and well-defined with a high degree of central concentration. The light distribution suggests a primarily spheroidal structure, lacking prominent spiral arms or a discernible disk component. The color profile is consistent with an evolved stellar population, exhibiting a yellowish-red hue, indicative of older, cooler stars dominating the light output. There is no evidence of recent or ongoing major mergers or significant tidal disturbances; the galaxy appears relatively undisturbed. The overall impression is that of a passively evolving system.
