The galaxy appears to be a relatively small, elliptical galaxy at a moderate redshift. It exhibits a smooth, centrally concentrated light profile with no apparent spiral arm structures. There is an elongation to the galaxy, with the aspect ratio suggesting that it is somewhere between a round and cigar shape. The color is a somewhat homogenous yellow-white, potentially indicating an older stellar population with relatively low ongoing star formation. There are no visually apparent signs of active galactic nuclei activity, strong dust lanes, or major merger events. Slight irregularities in the outer regions of the galaxy could point to minor past disturbances but do not appear significant.
