This galaxy presents a relatively smooth, elliptical morphology, although some slight irregularities suggest potential disturbances or faint features within its structure. The galaxy is dominated by a redder, more centrally concentrated core, indicative of an older stellar population. Surrounding this core, there is a more diffuse and slightly bluer halo, hinting at the presence of younger stars or ongoing star formation, albeit at a seemingly low rate. The overall shape appears to be somewhat rounded, showing no strong signs of a disk structure. There are possible interactions with a companion galaxy, or even internal activity or past mergers could be affecting the structure. The relatively smooth appearance suggests it is in a later stage of merging or has largely settled following a disturbance. The size suggests a moderately large galaxy, with its light extending a few kiloparsecs.
