This galaxy appears to be a relatively undisturbed system, likely a lenticular or early-type spiral galaxy seen at a distance where finer details are blurred. It exhibits a smooth, elliptical morphology, with a noticeable central bulge that appears bright and concentrated. There is a clear color gradient, transitioning from a yellowish-white core to a redder halo region. This suggests an older stellar population dominates throughout, with a possible decline in star formation activity. No prominent spiral arms, dust lanes, or tidal features are immediately discernible. The galaxy's overall form indicates a system that is well-evolved and dynamically settled, with little evidence of recent mergers or significant interactions. The roundness of the galaxy suggests it is an elliptical galaxy more so than a spiral.
