The galaxy presents as a relatively smooth, elliptical morphology, with a high degree of central concentration. The galaxy exhibits a slight elongation. The core appears a more yellow-red hue, while the outer regions have more green coloring. The light distribution suggests that the galaxy is dominated by an evolved stellar population, particularly in the central bulge region. The outer regions appear bluer, but with a relatively old population of stars, suggesting less star formation activity. There is no evidence of significant dust lanes or spiral arm structure. Overall, it appears to be a well-formed, relatively undisturbed galaxy in a late stage of evolution.
