The galaxy presents a generally smooth, elliptical morphology. It exhibits a high degree of central concentration with a bright, well-defined core. The galaxy appears largely featureless, lacking prominent spiral arms or distinct dust lanes. The color profile suggests a dominant population of older stars, indicated by its reddish-yellow hue, which is likely due to the presence of evolved red giant stars. There is little indication of ongoing, significant star formation activity based on its color and smooth texture. The overall shape is somewhat elongated, deviating slightly from a perfectly circular form. The galaxy does not show any obvious signs of major mergers or tidal disturbances, suggesting a relatively undisturbed evolutionary history. There is a faint halo surrounding the core, gradually fading into the background.
