The galaxy presents as an elliptical morphology, appearing largely smooth and relatively featureless. The light profile suggests a concentrated spheroid, lacking prominent spiral arms or a well-defined disk structure. There is a suggestion of a slight elongation, though the overall shape is predominantly round. The color gradient appears to be relatively uniform across the galaxy, with a yellowish-orange hue dominating. This may indicate an older stellar population and suppressed star formation, suggesting a galaxy that has largely exhausted its gas supply or whose gas has been heated such that it is no longer collapsing into stars. There are no obvious signs of recent or ongoing mergers, tidal tails, or strong disturbances in its overall structure and a lack of strong blue light.
