The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing yellowish, possibly indicating an older stellar population. The light gradually diffuses outwards, transitioning to a greenish hue in the outer regions. This coloration could be indicative of ongoing, but limited, star formation within the disk. There is no visible evidence of a prominent disk structure, spiral arms, or a bar. Nor is there any strong indication of tidal tails or other disturbances indicative of recent major merger activity. There are no obvious indications of active galactic nuclei activity. Overall, the galaxy appears as a relaxed, evolved system with a modest amount of on-going star formation.
