The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge that transitions into a more diffuse halo. The core exhibits a yellowish-orange hue, suggesting an older stellar population and lower rates of current star formation. Surrounding the core, there is a greenish-blue aura that may be indicative of some ongoing, albeit limited, star formation or perhaps emission from ionized gas. There is no clear evidence of spiral arms or a distinct disk structure. The overall morphology suggests the galaxy may be undergoing, or has undergone, a minor disturbance, but is generally undisturbed.
