This galaxy presents as a somewhat elongated, elliptical morphology. The central bulge exhibits a high surface brightness with a yellowish-orange hue, indicating a likely older stellar population. Moving outwards, the galaxy exhibits a gradual decrease in surface brightness, transitioning into a fainter, more diffuse halo. Hints of disk features can be seen. The disk has a bluer hue, suggesting the presence of younger stars and ongoing star formation. There are no indications of strong spiral arm structure.

Overall, the galaxy appears to be relatively undisturbed, with no signs of major mergers or tidal interactions. Minor disturbances or features cannot be excluded, although they are not readily apparent. Based on its colors and morphology, this galaxy is likely a massive system undergoing moderate levels of star formation.
