The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. There's a distinct, bright, yellowish core region indicating a likely concentration of older stars. Moving outward from the core, the color transitions to a more reddish hue, possibly indicating a less active star formation rate in the outer regions. No clear spiral arm structures or significant dust lanes are apparent. The overall structure suggests a relatively quiescent galaxy, potentially an early-type galaxy that has largely exhausted its gas supply for active star formation. There is no evidence of tidal disturbances or ongoing mergers.
