The galaxy exhibits a largely smooth morphology, appearing elliptical in shape, though not perfectly round, showing a slight elongation. It displays a central concentration of light that diminishes gradually outwards. There are subtle indications of faint, diffuse features surrounding the core. Overall, the galaxy presents as a relatively undisturbed system, with no obvious signs of significant tidal interactions or major mergers in its recent history. The color profile suggests a population of older stars, exhibiting a relatively redder hue.
