The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high surface brightness with a yellow-orange hue, suggestive of an older stellar population. Moving outward from the core, the light gradually diffuses, with a subtle blue tinge appearing in the outer regions. This could indicate the presence of younger, hotter stars within the galaxy's halo. There's no clear evidence of spiral arms or prominent dust lanes. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. It appears well-defined. Overall, the galaxy seems to be a fairly massive and luminous system.
