The galaxy appears as a moderately bright, centrally concentrated object. Its overall shape is elliptical and largely smooth, with a subtle disk-like structure apparent. The central bulge is prominent and exhibits a yellowish-white hue, suggesting an older stellar population. The disk shows hints of bluer color indicative of younger stars, though star formation activity appears subdued across the galaxy. There is no evidence of significant spiral arm structure or major disturbances, but there are some slight asymmetries present, which may indicate a minor recent interaction or merger.
