The galaxy exhibits a generally elliptical morphology with a bright, concentrated central bulge. The bulge appears yellowish-white, suggesting an older stellar population. A fainter, diffuse disk surrounds the bulge, displaying a subtle bluish tint that implies the presence of some younger, hotter stars and ongoing star formation, albeit at a relatively low rate. The galaxy appears relatively undisturbed, lacking obvious signs of major mergers or tidal interactions. The overall smoothness and lack of prominent spiral arms suggest a relatively evolved system, with a significant fraction of its stellar mass already formed. The galaxy's color gradients indicate a radial variation in stellar population, with older, redder stars concentrated in the center and younger, bluer stars more prevalent in the outer disk.
