The galaxy presents a largely elliptical morphology, appearing quite smooth in structure. The central region exhibits a high degree of concentration and a yellowish hue, suggesting an older stellar population dominates its composition. There is some indication of a very faint, diffuse halo extending outwards from the core. There is no visual evidence of spiral arms or significant dust lanes. The galaxy's apparent color suggests it is dominated by relatively old stars with low rates of star formation. Overall, it appears to be a fairly evolved galaxy without any obvious signs of recent mergers or active galactic nuclei activity. The light emitted is likely a redshift, meaning the galaxy is at quite a distance from us.
