The galaxy appears to be a relatively smooth, elliptical type. Its light is concentrated towards the center in a bright, unresolved core which may contain a supermassive black hole. There is a gradual fading in luminosity as you move outward from the core towards the edges of the galaxy which means the stars have an even distribution and it has a fairly simple structure. The main body has a slightly oblong shape which could mean that it is slowly colliding with another, smaller dwarf galaxy. The galaxy exhibits a subtle color gradient, appearing slightly bluer near the core, suggesting a region of moderate star formation activity, and more red on the outskirts, pointing towards an older stellar population. This could indicate the younger stars are closer towards the center, while the redder and older stars are on the outer edges. Overall, the system appears relatively undisturbed, lacking any major signs of recent mergers or tidal interactions.
