The galaxy presents as a largely smooth, elliptical structure with a concentrated central bulge. There's a gradual fading of luminosity from the core outwards, with no distinct spiral arm features visible. The color distribution appears relatively uniform, with a slightly redder central region suggesting an older stellar population, and a hint of bluer hues in the outer regions, which might indicate ongoing, though low-level, star formation. There's no evidence of strong tidal interactions or major disturbances in its morphology, suggesting it is likely a relatively isolated system. The galaxy's shape is mostly circular, exhibiting little ellipticity, with a subtle extension along one axis. Overall, the galaxy appears as a mature, early-type system.
