The galaxy presents an overall smooth morphology, appearing as an elliptical or spheroidal structure. There is minimal indication of spiral arms or a distinct disk component within the visible light. Its shape tends to be a rounded, with a slight elongation. The color distribution appears relatively uniform across the galaxy, with a dominant reddish hue. This suggests an older stellar population. There is a hint of potential interaction or merger event due to minor disturbances in its structure.
