The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features suggestive of active star formation regions. The galaxy exhibits a noticeable color gradient, transitioning from a yellowish-white core to a redder halo. This color variation could indicate variations in stellar populations, with older, redder stars dominating the outer regions and a population of younger and bluer stars in the central region. The overall appearance suggests a relatively evolved system with minimal ongoing star formation. There appears to be a slight asymmetry in the outer halo, which could suggest minor tidal interactions or past merger events, but the overall structure is largely undisturbed.
