This galaxy exhibits a notable central bulge, appearing relatively smooth and concentrated. The extended disk surrounding the bulge shows some subtle features, but lacks well-defined spiral arm structures. The light distribution appears asymmetric, with slightly more extended emission on one side. The galaxy's color is generally yellowish, suggesting an older stellar population, though some bluer regions indicate ongoing star formation. There are no obvious signs of strong tidal interactions or major mergers, although subtle disturbances in the outer regions may indicate minor past interactions. Overall, the galaxy appears to be in a relatively stable state, transitioning from a more active to a quiescent phase of evolution.
