The galaxy presents as a largely smooth, elliptical morphology. It exhibits a high degree of central concentration of luminosity, transitioning outward to a fainter, more diffuse halo. The color profile suggests a relatively old stellar population, dominated by redder wavelengths, with only a slight hint of bluer light in the core. There is no obvious disk structure, spiral arms, or significant dust lane features visible in this image. The general appearance points toward a quiescent system with potentially low current star formation activity, and no clear signs of a recent or ongoing major merger event or tidal disturbances.
