The galaxy presents a largely smooth, elliptical morphology with a central bulge exhibiting a yellowish-white hue, suggesting a population of older stars. The overall shape appears to be somewhat elongated, possibly deviating slightly from a perfect sphere. A faint blue halo surrounds the central region, potentially indicating regions of younger star formation. There's a hint of minor disturbance in the outer regions; however, no distinct tidal tails or bridges are apparent. The galaxy appears relatively isolated, with no immediately obvious signs of a major ongoing merger, though a close inspection of higher-resolution data may reveal finer details.
