The galaxy presents as a largely featureless, elliptical morphology with a high degree of central concentration. The light distribution appears smooth and centrally condensed, with a lack of distinct spiral arms or significant dust lanes. The color profile suggests a dominance of older stellar populations, given the relatively redder hue. There may be some slight indications of a very faint, diffuse disk, however the smooth nature indicates it is likely an elliptical galaxy. There does not appear to be any significant merging or tidal disturbances. The shape of the galaxy appears to be fairly round. There is low star formation.
