The galaxy presents as a relatively smooth, centrally concentrated object with an apparent red-shift. It displays a notable red color, indicating an older stellar population, possible dust obscuration, or a high redshift. The galaxy exhibits a slightly elliptical morphology, with its light distribution appearing predominantly uniform and lacking significant substructure such as spiral arms or distinct star-forming regions. There are only minor indications of tidal disturbances or interactions with neighboring galaxies, suggesting the galaxy is relatively isolated or in a late stage of merging. The shape is neither perfectly round nor highly elongated, instead, it takes a middle-ground elliptical structure. From the smooth structure, it has features typical of an elliptical galaxy type.
