The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth luminosity profile. The core exhibits a bright, yellowish hue, suggesting a population of older stars. The light gradually fades outward, transitioning to a redder color in the outer regions, which may indicate an aging stellar population with lower rates of recent star formation. There is a slight asymmetry observed, suggesting it is possibly interacting or may have undergone a minor disturbance in its past. There's no evidence of strong spiral arms or prominent dust lanes visible in this image. The general morphology points towards a galaxy that is relatively evolved, with a significant fraction of its stellar mass already formed.
