The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, with a high degree of roundness. The core region is bright and appears yellowish-white, indicative of an older stellar population. There's a gradual decline in luminosity moving outward from the center, fading into the surrounding background. There is no clear evidence of spiral arms or a disk-like structure. No significant tidal distortions or signs of ongoing major mergers are apparent. The overall color suggests a lack of substantial recent star formation activity.
