The galaxy presents as a centrally concentrated spheroid with a smooth light distribution. There is a high degree of radial symmetry and very little evidence of spiral arms or a disk. The color gradient indicates an older stellar population concentrated in the core, which transitions to a younger, bluer stellar population further from the center. There's no clear evidence of an active galactic nucleus or significant dust lanes within the visible spectrum, though such features may be obscured by distance or limitations of image resolution. There is some indication of minor disturbances in the outer regions. The surrounding halo lacks distinct features, though subtle variations in color suggest varying stellar densities, with the blue component representing regions of active star formation.
