The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, centrally concentrated light distribution. It is elliptical in shape, with a high degree of roundness. The galaxy displays a central bulge that dominates the overall structure. There is a subtle hint of a disk, but no clearly defined spiral arms are visible. The color is generally redder, suggesting an older stellar population with minimal ongoing star formation. There is no apparent sign of significant tidal disturbances or ongoing merger activity. The overall morphology suggests a relatively quiescent galaxy that is undergoing passive evolution.
