The galaxy presents as a relatively smooth, centrally concentrated object with a yellowish hue. The light is tightly bound to the center of the galaxy. There is no obvious spiral structure or prominent disk. The galaxy appears to be generally round in shape, without any significant elongation or distortions indicative of recent major mergers. There may be minor disturbances or irregularities. The galaxy lacks a dusty component as well as indications of significant ongoing star formation.
