The galaxy presents with an overall elliptical morphology, displaying a moderate degree of central concentration. The core region exhibits a bright, relatively smooth appearance with a distinct cyan-blue hue, suggesting active star formation or a dominant population of young, hot stars. There may be the presence of an Active Galactic Nucleus (AGN) contributing to the bright, blue appearance of the core. 

Moving outward from the core, the galaxy transitions to a more diffuse, less structured form. There are hints of possible tidal features or minor disturbances in the outer regions, potentially indicating past or ongoing interactions with other galaxies, however the resolution is fairly low. The outer regions are redder in color than the core, possibly due to the presence of older stellar populations or dust obscuration. The shape and structure of the galaxy appears significantly perturbed relative to more typical elliptical systems.
