The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that transitions smoothly into a broader, less dense halo. The galaxy has a slightly elongated shape, with its major axis oriented approximately horizontally in the frame. The light distribution is centrally concentrated, indicating a dominant, spheroidal stellar population. There is a relatively uniform color gradient, trending toward redder hues in the central regions and slightly bluer tones in the outer parts of the galaxy, suggesting that the central regions are dominated by older stellar populations, while the outer parts have more recent star formation. No distinct spiral arms or prominent dust lanes are visible. There are hints of possible minor disturbances or tidal features, with small amounts of asymmetric light distribution in the halo. Overall, it is a fairly compact and passively evolving galaxy.
