The galaxy presents as a relatively smooth, centrally concentrated object with a mostly elliptical morphology. There is a slight elongation, but it appears quite round overall. The central bulge is prominent and exhibits a yellowish-orange hue, suggesting an older stellar population. Evidence of possible disturbances can be seen. The galaxy's light distribution is concentrated, with no obvious spiral arms or distinct features. The color profile indicates an older stellar population, consistent with a more quiescent system with a low star formation rate. There appear to be 2 bright spots in the image that are likely either the core or artifacts of the image. It is difficult to ascertain whether this system is undergoing a major merger.
