The galaxy presents a generally smooth, elliptical morphology. It is centrally concentrated with a bright core that gradually fades towards the outer regions, appearing almost spherical in shape.  The color gradient suggests an older stellar population, with a yellowish hue dominating the central region and transitioning to a slightly bluer color in the outskirts, possibly indicating the presence of some younger stars. The galaxy shows no obvious signs of spiral arms or significant dust lanes. There is no apparent major disturbance to its structure, suggesting that this galaxy has not undergone a major merger recently. Overall, the galaxy appears to be a relatively quiescent system with ongoing, albeit low, star formation.
