The galaxy presents a generally smooth, elliptical morphology. There is a noticeable concentration of light towards the galactic center, which exhibits a yellowish hue, potentially indicating a population of older, less massive stars. Fainter, bluer light is distributed around the core, possibly suggesting some ongoing, albeit low-level, star formation. No spiral arm structures or strong dust lanes are discernible within this image. The overall appearance indicates a well-formed system without significant signs of recent mergers or major tidal disturbances. The galaxy appears relatively isolated.
