The galaxy presents a largely smooth, elliptical morphology. It displays a concentrated central bulge, appearing yellowish-white, suggesting an older stellar population. The overall shape is somewhat elongated, but not drastically so, trending towards a more spheroidal form. There are no readily apparent spiral arms or dust lanes, which reinforces the interpretation as an elliptical or lenticular galaxy. A faint, diffuse halo of light is potentially observable, however the image resolution limits a comprehensive assessment of extended structure. The color profile indicates a possible red-sequence galaxy with low star formation activity. Minor distortions are subtly observed, suggesting that it could have had minor disturbances, or potentially have been part of a smaller merger in its past.
