The galaxy appears as a single, relatively smooth object. Its morphology is largely elliptical, exhibiting a high degree of circular symmetry. There is no obvious spiral structure or significant disk component visible. A slight elongation is perceptible, hinting at a possible deviation from perfect sphericity. The light is centrally concentrated, with the intensity decreasing gradually towards the edges. The galaxy's color profile shows a predominantly reddish-yellow hue, with a hint of green. Given the redshift, this coloration suggests an older stellar population. There are no immediately obvious signs of major disturbances or ongoing mergers. The object appears to be a well-formed, relatively quiescent galaxy.
