The galaxy appears to be a relatively smooth, elliptical system with a concentrated central bulge. Its color is yellowish-orange, suggesting an older stellar population with a lower rate of ongoing star formation. The galaxy exhibits a subtle elongation, deviating slightly from a perfect circular shape. There might be a faint, diffuse halo surrounding the main body, but the signal is weak. No prominent spiral arms or distinct features are readily visible. The overall morphology indicates a system that is likely quiescent and has undergone significant evolution. There are no signs of major mergers or tidal disturbances, but the galaxy might exhibit a slight interaction.
