This galaxy appears to be a relatively smooth, elliptical-like system. There is a central, bright, and somewhat diffuse region, which could be the galactic bulge or core. The light profile appears to decrease steadily moving outward from this center, with no obvious spiral arm structures or significant dust lanes visible. The color gradient suggests a slightly bluer central region, possibly indicating younger stellar populations there, grading to redder hues in the outer regions. The overall shape is elongated, rather than perfectly spherical, but it doesn't exhibit any major disturbances, tidal tails, or signs of a major ongoing merger. The faintness and size indicate that we are looking at a galaxy some ways away.
