The galaxy presents as an elliptical morphology, with a smooth, featureless appearance. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. A bright, yellowish core is apparent, suggestive of an older stellar population. The overall color of the galaxy exhibits a subtle gradient, transitioning from the yellowish core to a slightly bluer hue in the periphery, potentially indicating the presence of some younger stars or residual star formation in the outer regions. There is no discernible evidence of spiral arms, dust lanes, or ongoing major merger activity. The shape is close to round but slightly elongated. Faint disturbances are possible but not overtly visible.
