The galaxy presents as a generally smooth, elliptical or lenticular system. It exhibits a concentrated, bright central bulge transitioning outward to a less luminous and more diffuse halo or disk component. The core is notably yellowish-orange. The lack of defined spiral arms or dust lanes suggests a relatively quiescent system, consistent with a classification towards the red sequence. There is no evidence of significant ongoing star formation visible in the image, further supporting the observation of a primarily evolved stellar population. The galaxy appears relatively isolated, lacking obvious signs of interaction or tidal disturbances, but there are some faint points of light in its general vicinity. Given the galaxy's redshift, any fine details are not discernible in this image.
