The galaxy presents as a relatively smooth, elliptical-like object with a concentrated central bulge. The color profile suggests a dominant population of older stars, indicated by the reddish-orange hue, particularly in the central region. There is evidence of some bluer light in the surrounding regions, possibly indicating ongoing, although subdued, star formation relative to the core.

There is a slight asymmetry in the outer regions, hinting at potential minor gravitational interactions or internal dynamics, but overall the galaxy appears largely undisturbed. Its shape is neither perfectly spherical nor highly elongated, exhibiting an intermediate ellipticity.
