The galaxy appears to be a relatively smooth, elliptical type. It has a concentrated central bulge that is a yellow-orange hue, suggesting an older stellar population. This central region fades gradually into a more diffuse halo. There are no readily apparent spiral arms or dust lanes visible in this image. The galaxy's overall shape is roughly circular, with only slight deviations from perfect roundness. Based on the lack of distinct features, it is likely undergoing little to no active star formation. There is no evidence of a recent or ongoing merger.
