The galaxy presents a primarily elliptical morphology, appearing significantly rounded in shape, although exhibiting a slight elongation, suggesting a classification somewhere between perfectly spherical and cigar-shaped. The central bulge is prominent and displays a yellowish-orange hue, indicative of an older stellar population. A faint, bluish disk surrounds the bulge, hinting at the presence of younger stars and possibly ongoing, but subdued, star formation. There is no obvious spiral structure, though a subtle mottled texture in the disk suggests some irregularities. No major signs of interaction or merging activity are apparent, with the galaxy displaying a relatively undisturbed structure. Overall, the galaxy appears to be a massive system that is largely quiescent in terms of star formation, though it doesn't completely lack in star formation activity.
