The galaxy presents as an elliptical morphology with an intermediate roundness, appearing neither perfectly spherical nor particularly elongated. There is a smooth profile, but there is a possible hint of a disk. The galaxy exhibits a color gradient, appearing redder and brighter towards the core and fading to green hues towards the edges, which could suggest ongoing star formation. The central bulge appears prominent and well-defined. There appears to be no major disturbance due to any mergers with another object, indicating that the galaxy is in a relatively settled state.
