The galaxy presents a generally elliptical morphology with a high degree of smoothness. The core exhibits a concentrated, bright yellow-orange hue suggesting an older stellar population. The surrounding region appears less concentrated with a gradual fading in intensity and shift toward slightly redder tones toward the galaxy's periphery. There is little indication of distinct spiral arm structures or significant dust lanes and no obvious signs of active galactic nuclei based on the image alone. A slight asymmetry can be seen in the halo structure, though no significant merger is visible. It appears to be a relatively undisturbed galaxy, and possibly, given the color, an older galaxy.
