The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that is nearly circular in appearance. The color profile indicates a generally older stellar population, with a dominant yellowish hue suggesting a paucity of active star formation within the galactic body. There are hints of a very faint, diffuse halo extending outward from the main structure, which may indicate prior minor merger events or gravitational interactions. Overall, the galaxy appears relatively undisturbed.
