The galaxy presents as an elliptical morphology, with a high degree of central concentration. The light profile appears smooth and largely featureless, lacking discernible spiral arms or a prominent disk structure. The color gradient suggests a redder core transitioning to a slightly bluer outer halo. This might indicate an older stellar population in the central region, with some younger, bluer stars residing in the outskirts. There appears to be ongoing, but low, star formation activity. It appears to be relatively undisturbed, showing no signs of recent major mergers or tidal interactions.
