The galaxy presents as an elliptical morphology, exhibiting a smooth, diffuse light distribution. The light is more concentrated at the center, growing fainter in intensity as it extends away from the center. There appears to be no presence of spiral arms, bar structures, or significant dust lanes. The galaxy's color profile suggests a slightly red hue, becoming increasingly red towards the central region. There is a faint, broad, and diffuse disk that is greenish in color. The elliptical form is consistent with it being an older galaxy exhibiting low star formation. There are no apparent signs of recent merger activity or significant tidal disturbances in the visible light.
