The galaxy presents as a somewhat amorphous, though generally rounded, structure. The light profile appears relatively smooth and centrally concentrated, hinting at a dominant spheroidal component. However, there's a subtle elongation, deviating slightly from a perfect circle. The galaxy does not appear completely isolated; subtle disturbances or faint tidal features are not obviously absent in the image. These could indicate past or ongoing gravitational interactions. There is some visual evidence of disruption in the overall shape. The central region exhibits a brighter, compact core. The color appears to be a fairly uniform light blue across the main body of the galaxy. There is no obvious strong evidence of pronounced spiral arms or significant dust lanes are visible. This overall morphology suggests that the galaxy could be a early-type galaxy.
