This galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that appears nearly spherical and is comprised of a high density of stars. Moving outward from the core, the stellar density decreases, transitioning into a more diffuse halo. There is a slight elongation in the shape of the galaxy; it is more lens-shaped than perfectly spherical. The galaxy is a blue-white hue overall, with the core having a higher concentration of white light, and the halo taking on a bluer tone, suggesting ongoing star formation. There is no visible spiral arm structure or significant dust lanes. Based on its morphology, this galaxy is likely a massive system with a high stellar mass and a moderate rate of star formation. There are no signs of any major galactic mergers or interactions; the galaxy appears to be a relaxed system.
