The galaxy presents as an elliptical or lenticular type, displaying a largely smooth, featureless structure. The core exhibits a concentration of luminosity, possibly indicative of an active galactic nucleus or a high density of stars. The galaxy appears mildly elongated. There is a very subtle color gradient, transitioning from a slightly bluer hue in the central region to a redder tone towards the outer edges. No distinct spiral arms or prominent dust lanes are discernible, confirming the lack of significant ongoing star formation. The overall morphology suggests a gravitationally settled system, likely a mature galaxy that has undergone significant evolutionary processes. No clear signs of any recent or ongoing mergers can be seen.
