The galaxy presents as a relatively smooth and rounded elliptical morphology. There is a distinct central bulge that dominates the galaxy's luminosity. The color profile suggests an older stellar population. The galaxy exhibits a general lack of defined spiral arms or prominent dust lanes, indicating a lack of significant ongoing star formation. There are no obvious signs of tidal disturbance or interaction with other galaxies. The light is concentrated in the center, decreasing outward, with very little disc structure.
