The galaxy presents a primarily smooth morphology, appearing as a flattened elliptical or a lenticular galaxy viewed at an oblique angle. Its overall color is yellowish-white, suggesting a population dominated by older stars. There is a slight concentration of light towards what appears to be the galaxy's center, but no distinct nucleus is visible. Hints of bluer regions exist toward the outer edges, potentially indicative of ongoing, albeit limited, star formation within a disk component. Subtle distortions in the overall shape suggest a history of minor gravitational interactions.
