The galaxy appears to be elliptical in shape, with a smooth, concentrated central bulge. The color gradient suggests an older stellar population, with a yellow to reddish hue dominating the central region. There are two regions on either side of the bulge that appear to be star forming regions, with relatively small concentrations of more active stars. The overall structure exhibits signs of a possibly post-merger environment, with some minor disturbances visible in the outer regions. While the core is concentrated, the galaxy does have a relatively large radius overall.
