The galaxy presents a generally smooth, elliptical morphology, though there is some evidence of internal structure. The primary light is concentrated in a central bulge region, which appears to be a golden color. This bright central region transitions to a more diffuse reddish outer halo. There appears to be a flattened disk structure that is nearly edge-on, indicated by the ellipse shape of the galaxy. There are some bluer regions along the outer edges of the disk, suggesting the possibility of some star forming regions. There does not appear to be any major disturbances or significant merger activity present, though there may be a very slight asymmetry to the halo, suggesting a minor interaction in the past. The overall appearance suggests a relatively evolved system.
