The galaxy appears as a somewhat smooth, elliptical structure with a bright, concentrated central bulge. The color profile suggests an older stellar population, with a yellow-red hue dominating the core and inner regions. There are hints of a faint, extended halo surrounding the central region, though its boundaries are poorly defined.  No obvious spiral arm structures or significant dust lanes are visible.  The overall morphology suggests a relatively evolved system, possibly in the process of quenching star formation. There are no obvious signs of major mergers or tidal disturbances, although some minor asymmetry may exist in the outer regions, potentially indicating past interactions.
