The galaxy appears to be a relatively smooth system, with a dominant spheroidal component. It exhibits a moderate ellipticity, appearing as a flattened spheroid rather than perfectly circular. There's a hint of a disk structure embedded within the bulge, but it is not prominently defined. The light distribution suggests that the bulge dominates the overall morphology. No prominent spiral arms are visible. It has a redder color than the other objects in the image, and looks like a somewhat evolved galaxy that is no longer forming many stars. The galaxy shows no obvious signs of major disturbances or ongoing mergers, though subtle irregularities in its shape could indicate minor past interactions.
