The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and rounded morphology. The light distribution is centrally concentrated, showing a gradual decrease in intensity outwards. The core region is brighter, suggesting a higher density of stars. There's a subtle color gradient, with the central region exhibiting a slightly redder hue compared to the outer regions. The overall structure lacks distinct spiral arms or a prominent disk, implying a relatively old stellar population with minimal recent star formation. There are no signs of significant tidal distortions or ongoing mergers.
