The galaxy presents as an elliptical morphology, with a smooth, relatively featureless light distribution. The core region exhibits a high degree of luminosity, appearing bright yellow/orange. The light gradually decreases toward the edges, appearing more green and then darkening, suggesting a diminishing stellar density in the outer regions. The overall shape is somewhat elongated, though predominantly spheroidal, showing a slight cigar-shaped appearance. No distinct spiral arms or bar structures are discernible within the resolution limits. The smoothness of the galaxy suggests a later-type system that has likely undergone significant merging or lacks substantial ongoing star formation. There is no evidence of active galactic nuclei activity, tidal tails, or ongoing major merger events within this image. Faint blue-green gradients around the perimeter might indicate the presence of low-level star formation or a population of younger stars, though this is difficult to ascertain due to the lower resolution.
