The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. Its color profile suggests an older stellar population, with a dominant yellow-orange hue, transitioning to redder tones in the outer regions. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy exhibits a fairly uniform surface brightness, with a gradual decrease in luminosity from the core outwards. No signs of active galactic nuclei or significant star formation regions are visibly apparent within the galaxy's structure, and it appears to be relatively undisturbed with no major merger events. It is moderately massive.
