The galaxy appears to be a single, relatively smooth object with a concentrated central bulge that emits strongly in the redder wavelengths. The galaxy presents an elliptical morphology. There is no clearly defined disk structure visible, nor any prominent spiral arms or dust lanes. A very slight elongation is observed, with no clear signs of ongoing or recent major merger activity that would significantly disrupt the overall structure. There are no easily discernible tidal tails or other obvious features indicative of strong gravitational interactions. The light appears to be dominated by older stellar populations.
