This galaxy appears to be a relatively smooth, elliptical system. Its light profile exhibits a strong central concentration, with luminosity decreasing gradually towards the outer edges. There is little evidence of spiral arms or significant dust lanes. The color gradient suggests an older stellar population throughout much of the galaxy, with a slightly bluer hue at the outskirts implying the presence of younger stars in the surrounding regions. Overall, the galaxy appears largely undisturbed, with no obvious signs of a recent major merger or strong tidal interactions.
