The galaxy presents an overall elliptical morphology, appearing moderately elongated. Its color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue concentrated toward the galactic center. The outer regions show a faint bluish tint which could possibly indicate younger stars or low-level star formation, although this is subdued. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy appears relatively undisturbed, showing no obvious signs of a major merger or significant tidal interactions. There may be minor disturbances present, but nothing substantial.
