The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The light profile is relatively uniform, lacking any discernible spiral arm structures or prominent dust lanes. The color gradient appears to shift towards redder hues in the central regions, suggesting an older stellar population dominates the core. The outer regions exhibit slightly bluer tones, which may indicate the presence of some younger stars, though not in significant quantities. The galaxy appears relatively isolated, showing no signs of major tidal disturbances or ongoing mergers, though there could be a minor interaction. Overall, this galaxy appears to be a mature, quiescent system.
