The galaxy presents as a relatively smooth, elliptical-like structure. It appears roughly circular. The galaxy exhibits a color gradient, transitioning from a yellow-orange hue at its core to a bluer color on the edges. This suggests a possible difference in stellar populations between the central bulge and the outer regions of the galaxy, possibly due to recent star formation. There is a hint of minor asymmetry, which may indicate a previous merger or gravitational interaction. This is further supported by the irregular color distribution. The galaxy is relatively isolated, without any immediately apparent major companion galaxies or strong tidal features.
