The galaxy exhibits a largely elliptical morphology, appearing quite smooth and relatively featureless across its visible extent. It possesses a concentrated central bulge with a high degree of radial symmetry, decreasing in luminosity as distance from the center increases. There is some slight evidence of a faint disk-like structure or diffuse outer halo, but it is not sharply defined, the transition between bulge and disk or halo is gradual. There is no definitive evidence of spiral arms or bar structure within the observed wavelengths. The color profile suggests a population of older stars, giving it a yellowish to reddish hue. Indications of current significant star formation are absent in this image. There is no evidence of tidal tails or major disturbances indicative of recent major merger activity, with a slight possibility of minor interaction effects. The overall appearance aligns with a relatively evolved and quiescent galaxy.
