The galaxy presents a largely smooth, elliptical morphology. Its light is concentrated centrally, exhibiting a radial decrease in luminosity moving outwards from the core. The color profile appears relatively uniform across the galaxy, trending towards a redder hue. There are no discernible spiral arms, bars, or dust lanes. The overall structure suggests a spheroidal system with minimal ongoing star formation. There is some slight asymmetry, possibly indicating a past or ongoing minor interaction or disturbance, but it is difficult to make a definitive claim of merger activity. The galaxy appears quite round in shape.
