The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular type. Its shape appears somewhat elongated, with a moderate axis ratio. The central region exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a dense stellar population. The color gradient transitions from a yellowish-white hue in the core to a more muted blue towards the outer edges, potentially signifying older stellar populations in the center and younger stars in the periphery. Faint, diffuse extensions or tidal features may be present, hinting at possible past or ongoing interactions with other galaxies. Overall, the galaxy appears relatively undisturbed with only mild morphological distortions.
