The galaxy appears to be elliptical in morphology, exhibiting a smooth, concentrated light distribution. The core region is significantly brighter and more yellow than the outer regions of the galaxy, indicating a potentially older stellar population dominating the center. The galaxy exhibits a relatively high degree of central concentration and appears to lack any spiral arm structures or prominent dust lanes. The overall color profile suggests a red sequence galaxy, indicative of a passively evolving system with a low star formation rate. There are no visible signs of active galactic nuclei activity or major disturbances in the overall structure. The elliptical shape is slightly elongated, with an approximate axis ratio of 0.8.
