The galaxy presents a generally smooth morphology, appearing as a slightly elliptical structure. The central region is characterized by a bright, concentrated luminosity profile indicative of a significant stellar population. The galaxy exhibits a moderate redshift, suggesting that we are observing it at a considerable distance. It shows a relatively low star formation rate, its color is yellow and there is a hint of a blue edge. This suggests the galaxy is primarily composed of older stellar populations. There is no sign of recent or ongoing major merger events. However, there may be minor disturbances within the galactic structure.
