The galaxy presents a generally smooth, elliptical morphology, appearing relatively undisturbed. The light distribution suggests a high degree of central concentration. There is a noticeable color gradient, with the core exhibiting a yellowish-white hue, indicative of an older stellar population. The outer regions are slightly bluer, suggesting the presence of some younger stars, although the overall star formation rate appears relatively low. There is a faint disk that is observed along the edges of the galaxy, with a very slight tilt. No prominent dust lanes or spiral arm structures are readily apparent in this image. The galaxy's shape is quite round, with only a slight elongation. There may be some very minor disturbance or interaction occurring, though the galaxy is generally very uniform.
