The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. It lacks prominent spiral arms or a well-defined disk structure. The light profile suggests a spheroidal shape with a relatively high degree of roundness. Color gradients are subtle, with a slightly redder core region transitioning to marginally bluer outer regions. There is no apparent evidence of ongoing major mergers or significant tidal disturbances. The galaxy is likely in a relatively quiescent state, with a moderate stellar mass and a relatively low rate of star formation.
