The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge, appearing yellowish-white, dominates the core region. This suggests an older stellar population. The overall shape is consistently rounded, with no obvious elongation or asymmetries. There is a faint, diffuse halo extending outward from the core, exhibiting a bluer color than the central bulge. It is likely that this halo contains small amounts of younger stars and some ongoing star formation. No distinct spiral arms, bars, or other features suggestive of a disk component are visible. There is no visually apparent evidence of ongoing or recent major mergers or tidal disturbances. Overall, the galaxy shows characteristics consistent with a relatively quiescent system that has largely completed its major star-forming epoch. The overall red shift confirms that this is not a local galaxy.
