This galaxy appears to be in the process of merging. The primary, larger component exhibits a relatively smooth, elliptical morphology, with a concentrated central bulge that emits strongly. A smaller, less distinct component is visible in close proximity, displaying a less regular shape. This second component seems to be disrupting the symmetry of the primary galaxy. There appears to be a bridge of material connecting the two. The overall color of the system suggests an evolved stellar population, with a higher proportion of older, redder stars. There are no clearly defined spiral arms present. The system displays a moderate luminosity.
