The galaxy presents as a primarily smooth, elliptical structure. It exhibits a color gradient, appearing slightly redder towards the core and transitioning to a bluer hue in the outer regions. This suggests a central population of older, redder stars and younger, bluer stars in the outskirts, hinting at ongoing, though perhaps subdued, star formation activity. There is a subtle elongation visible in the galaxy's shape, with a relatively round morphology, suggesting it is not a highly distorted system. There is no strong indication of tidal tails or significant merger activity, but there are subtle disturbances.
