The galaxy presents as an elliptical morphology, exhibiting a generally smooth light distribution with a high degree of central concentration. The light profile appears relatively uniform without prominent spiral arms or bar structures. There is a slight deviation from perfect circularity, trending towards a more spheroidal shape. The color gradient suggests an aging stellar population, shifting towards redder wavelengths in the central regions and subtly bluer hues at the periphery, indicative of potentially ongoing, but low-level, star formation activity. The overall structure doesn't show significant signs of ongoing mergers or tidal disruptions, though there's a faint asymmetry that may warrant further investigation to rule out minor interactions or internal disturbances.
