The galaxy appears to be an elliptical galaxy. Its central region exhibits a high surface brightness, appearing nearly uniform and yellowish in color. This suggests a high concentration of older stellar populations. Moving outward from the center, the galaxy's light gradually fades, forming a more diffuse halo. This outer region seems largely smooth with a blue tint in portions of the galaxy. The overall shape of the galaxy appears approximately round, with no obvious spiral arm structures or significant dust lanes visible. There are no signs of ongoing major mergers or tidal disturbances are observed, suggesting a relatively isolated system or a system having completed any major merger events in its past.
