The galaxy presents a largely smooth, elliptical morphology. There is a concentrated central bulge with a yellow-orange hue, suggesting an older stellar population dominates the core. The galaxy exhibits a relatively uniform brightness distribution, indicative of a lack of prominent spiral arms or distinct features. There is a slight elongation, as opposed to a perfect circle, and a small concentration of light to the side of the main galaxy. The absence of strong blue colors suggests relatively low ongoing star formation activity within the galaxy. There does not appear to be any indication of interaction with a merging companion.
