This galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an overall elliptical morphology, with a significant degree of roundness, although it isn't perfectly spherical. There's no distinct disk structure visible. The color profile indicates a redder core region that transitions to a somewhat bluer halo. The smoothness suggests an older stellar population, with the redder core possibly indicating a higher concentration of older, evolved stars. There's no strong evidence of ongoing major merger activity, although there may be minor asymmetries, possibly indicative of a minor disturbance or past interaction. Overall, the galaxy seems to be a relatively massive, evolved system with suppressed star formation.
