The galaxy presents an overall elliptical morphology, exhibiting a moderately smooth structure in the central region. A bright, concentrated core dominates the luminosity profile, suggesting a significant concentration of stars and potentially a central supermassive black hole. Extending outwards from the core, a faint and diffuse halo is apparent.

There are some minor disturbances in the surrounding halo, indicating a possible history of gravitational interactions or mergers. The color gradients across the galaxy are subtle, but suggest a relatively homogenous stellar population. Specifically, the central region appears slightly redder compared to the outer halo. Overall, the galaxy seems to be in a relatively evolved state, with evidence of past disturbances but a currently stable, elliptical form.
