The galaxy presents a smooth, elliptical morphology. It exhibits a pronounced central bulge, characterized by a concentrated, bright luminosity. The overall color profile leans towards redder wavelengths, suggestive of an older stellar population. The shape appears elongated, exhibiting an intermediate ellipticity, falling between a perfect sphere and a cigar shape. There are no apparent signs of major disturbances or ongoing mergers; the galaxy presents a generally undisturbed structure. Faint, diffuse outskirts are observed, extending beyond the central, brighter regions.
