The galaxy presents as a relatively smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual decrease in surface brightness moving outward. The central region exhibits a bright, condensed core, possibly indicative of an active galactic nucleus or a dense stellar population. The overall color is slightly blue-white, which suggests a moderate amount of recent or ongoing star formation activity. No distinct spiral arms or bar structures are visible. There may be some evidence of minor tidal disturbance or faint, diffuse features in the surrounding halo, but these are not sharply defined.
