The galaxy presents a generally smooth, elliptical morphology. The central bulge region exhibits a concentrated, bright glow, transitioning outwards into a less intense halo. The shape of the galaxy leans towards round. There is no clear evidence of spiral arm structures or a prominent disk. The overall color of the galaxy is slightly redder, with a hint of yellow, suggesting an older stellar population and a low rate of star formation. No major distortions or merging features are readily apparent, implying the galaxy is relatively undisturbed. The galaxy appears to be isolated, with no other galaxies nearby that might suggest an ongoing interaction.
