The galaxy presents an overall elliptical morphology, with a smooth and largely featureless appearance. There is a concentration of light towards the galactic center. The color profile suggests a slightly evolved stellar population, as indicated by the orange/yellow hue dominating the central region. A faint, diffuse halo extends outwards from the core, gradually fading into the background. There are no clear indications of prominent spiral arms or ongoing major merging activity, although there are some minor perturbations in the outer regions.
