The galaxy appears to be a relatively smooth, elliptical system, exhibiting a centrally concentrated light profile. There is a bright, yellowish core that gradually fades into a less luminous, diffuse halo. The overall shape is neither perfectly spherical nor highly elongated, appearing somewhat in between. There's no clear evidence of spiral arms or a prominent disk structure. Minor distortions may be present, but the galaxy appears to be largely undisturbed, not showing signs of a major ongoing merger. The color is generally redder, indicating an older stellar population with relatively low ongoing star formation.
