The galaxy presents a largely smooth and elliptical morphology, exhibiting a concentrated central bulge that emits a yellowish-white light. The outer regions of the galaxy show a gradual decrease in luminosity, transitioning to a faint bluish hue. There is no prominent spiral arm structure or significant dust lane obscuration discernible from the image. The galaxy appears largely undisturbed, lacking evidence of ongoing major mergers or tidal interactions. It appears to be a fairly massive system, exhibiting a substantial rate of star formation. The overall shape is somewhat rounded, tending towards elliptical rather than a highly elongated form. There might be a faint disk structure imbedded within.
