The galaxy presents as a single, fairly homogenous structure. It exhibits a smooth, elliptical morphology with no discernible spiral arms or bar. There is a slight elongation, suggesting it is not perfectly spherical but leans more towards a rounded, but not cigar-shaped, appearance. The galaxy displays a radial color gradient, transitioning from a bright, yellowish-white core to a fainter, bluer outer region. This color difference indicates potential variations in stellar populations, with older, redder stars likely concentrated in the core and younger, bluer stars more prevalent in the outer regions, potentially indicating ongoing, but not extensive, star formation. There is no apparent evidence of major mergers or significant tidal disturbances. The general morphology suggests a relatively evolved system.
