This galaxy appears to be a relatively smooth, elliptical system. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population and possibly an active galactic nucleus. The galaxy's overall shape is somewhat flattened, deviating slightly from a perfect sphere.

There's subtle evidence of a disk-like structure, but the prominence of the bulge overshadows any distinct spiral arms. Faint extensions or tidal features are visible, potentially indicating past minor mergers or interactions. The color profile suggests a mix of stellar populations, with a yellow or green hue indicating the presence of intermediate to old stars. The overall smooth appearance suggests it is relatively relaxed system, possibly in a later stage of its evolution. 
