The galaxy presents a somewhat elliptical morphology. It exhibits a central bulge region that is brighter and more concentrated, surrounded by a more diffuse halo. The color gradient suggests a potentially older stellar population dominating the core, with a shift toward slightly bluer hues in the outer regions. While no distinct spiral arm structures are visible, there is an apparent slight flattening, suggesting a disk-like component. Based on the colors, the galaxy probably has low to moderate star formation activity. It appears relatively undisturbed with no signs of interaction with another galaxy.
