The galaxy exhibits a predominantly smooth morphology, with a concentrated central bulge that transitions into a fainter, more diffuse halo. The galaxy appears largely elliptical in shape, displaying a high degree of roundness. There's a hint of some internal structure beyond a purely smooth profile, though distinct spiral arms or a defined disk are absent. The core presents a yellowish-white hue, suggesting a population of older stars. Moving outward, the color shifts to include subtle blue and red tones, possibly indicating the presence of younger stellar populations and some dust. There is no apparent evidence of significant ongoing merger activity or major tidal disturbances. The overall appearance suggests this is a relatively evolved galaxy with a moderate level of star formation.
