The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that is bright and yellowish-orange in color, suggesting an older stellar population with a lower rate of star formation. The outer regions of the galaxy fade gradually, lacking distinct spiral arms or prominent features. There is a subtle color gradient, with the central regions appearing more yellow than the surrounding areas, which seem slightly redder, possibly due to dust obscuration. The overall morphology indicates that the galaxy is likely an evolved system, without significant ongoing mergers or interactions.
