The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile appears to diminish gradually from the core outwards, showing no distinct spiral arm features or prominent dust lanes. The color index suggests a population of older stars, with a yellow to orange hue in the central region. There is a hint of bluer light at the edges. The galaxy appears largely undisturbed with no signs of major mergers or tidal distortions.
