The galaxy appears to be relatively compact, with an overall elliptical morphology. The central region exhibits a bright, concentrated core, possibly indicating an active galactic nucleus or a dense stellar population. Moving outward from the core, the galaxy displays a smoother distribution of light, with a diffuse halo. There is a slight blue tint to the halo, which could indicate ongoing star formation. There are hints of some minor disturbances or irregularities in the outer regions, indicating possible past mergers or gravitational interactions, though these are not very significant. The galaxy appears to be generally smooth and lacks prominent spiral arms or a distinct disk-like structure.
