The galaxy appears as a moderately bright, centrally concentrated object with a generally smooth morphology. The galaxy exhibits a near-elliptical shape with a centrally located bulge that transitions smoothly into a surrounding halo. There is a color gradient, with the central region exhibiting a yellowish hue, potentially indicating a higher concentration of older stellar populations. The outer regions of the galaxy fade into a bluish-green tint, possibly suggesting the presence of younger, bluer stars. No distinct spiral arm structure or strong dust lanes are apparent. There might be some very slight disturbance in its otherwise smooth structure.
