The galaxy presents as a largely smooth, elliptical system. It has a concentrated, bright core that fades gradually outwards, with no apparent spiral arm structures or significant dust lanes visible. The color profile indicates a population of older stars, giving it a reddish-yellow hue. There is a slight elongation to the galaxy's overall shape, but it is generally round. No major signs of ongoing merger activity, such as tidal tails or distorted morphology, are immediately apparent, though minor disturbances cannot be entirely ruled out at this resolution. Overall, the galaxy appears to be a relatively quiescent system, potentially residing in a more evolved state.
