The observed galaxy presents a relatively smooth, elliptical morphology. The central region appears brighter and exhibits a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the core, the light gradually decreases in intensity. There is a slight elongation and asymmetry to the galactic structure. Patches of bluer light, likely indicative of areas of more recent star formation, are observed in some areas. There is no clear evidence of spiral arms or a distinct galactic disk. Overall, the galaxy shows minimal signs of significant disturbance or ongoing major merger activity.
