The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. The central region is brighter and appears more concentrated, fading outwards to less defined edges. There is a slight elongation to the overall shape, more 'in between' round than a perfect sphere.

The color profile appears yellowish-orange, suggesting an older stellar population dominating its composition. There may be some minor disturbances evident in the upper left, perhaps hinting at a minor interaction or past merger event. However, the overall structure is not heavily disrupted. The galaxy has a substantial mass. Star formation appears to be occurring, but at a relatively slow rate.
