This galaxy presents as a relatively smooth, elliptical structure. The central bulge is prominent and appears densely populated with stars, exhibiting a high degree of luminosity. Moving outward from the core, the stellar density gradually decreases, forming a diffuse halo that lacks distinct spiral arm features. The galaxy appears primarily quiescent with no notable dust lanes or active star-forming regions evident in this image, suggesting a population of older stars dominates its composition. The overall morphology is consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy seen at a moderate distance. There are no signs of tidal disturbances or ongoing mergers. It exhibits a slightly elongated shape, deviating marginally from a perfect circular form.
