The galaxy presents as a centrally concentrated elliptical type. It has a smooth, almost featureless morphology, lacking any prominent spiral arms or distinct disk-like structures. The light profile appears to be radially symmetric with a high degree of central concentration that gradually decreases with radial distance, but the shape looks slightly elongated, deviating from a perfect sphere. The color gradient transitions from a yellowish-white core to a dimmer, reddish-tinged periphery. There is no noticeable evidence of tidal disturbances, active galactic nucleus (AGN) activity, or ongoing major mergers. The galaxy appears relatively isolated and undisturbed. Overall, the galaxy is a quiescent system, likely dominated by an older stellar population with little ongoing star formation.
