The galaxy presents as a relatively compact, elliptical morphology. Its light profile is smooth and centrally concentrated, with a gradual decrease in intensity outwards. The color is generally consistent throughout the galaxy, exhibiting a slightly reddish hue, indicative of an older stellar population. There are no obvious spiral arm structures or prominent dust lanes visible. The overall form suggests a system that has undergone significant dynamical relaxation. It doesn't show any strong tidal features or signs of recent major mergers.
