The galaxy presents as a fairly smooth, centralized object. It exhibits an elliptical morphology, displaying an intermediate ellipticity, appearing neither perfectly round nor elongated. There is no obvious disk structure, nor any apparent spiral arm features.

The color profile indicates a population of older stars, as the galaxy's dominant hue is yellowish-orange. The even color distribution reinforces the idea of a galaxy with limited ongoing star formation.

There are no tidal tails or clear signs of a major merger event, though the faintest hint of asymmetry might imply a minor past interaction, or internal activity causing a slight disturbance.
