The galaxy presents as a singular, relatively smooth object with an elliptical morphology. The light profile is centrally concentrated, exhibiting a gradual decrease in intensity from the core outwards. There is minimal evidence of spiral arms or disk-like structures within the available imagery. The color appears generally uniform across the galaxy, with a subtle shift towards redder wavelengths, suggestive of an older stellar population. No obvious signs of recent major merger events or significant tidal disturbances are discernible. The roundness is in between a perfect circle and more cigar shaped.
