The galaxy presents a generally smooth, elliptical morphology, appearing as an oblate spheroid. The light distribution suggests a single component system with a centralized bright core region. The core appears concentrated and exhibits a yellowish-white hue. The outer regions of the galaxy fade into a more bluish color, suggesting the presence of some star formation relative to the central bulge, where older stellar populations likely dominate. There appears to be a very slight asymmetry to the galaxy, as there is a concentration of light towards the right edge. There are no clearly defined spiral arms or a prominent disk structure evident. Overall, the galaxy's light is relatively concentrated, with its half light radius being less than half of its overall radius.
