The galaxy presents a generally smooth morphology, with a high degree of central concentration. It appears elliptical in shape, with a subtle elongation. The light distribution appears relatively even across the galaxy. The color profile indicates a redder core, which subtly transitions to a bluer outer region. This potentially suggests an older stellar population concentrated towards the center, with the outer regions exhibiting more recent star formation activity. There are no distinct spiral arms, bars, or other clear morphological features that would indicate a disk galaxy. There are no obvious signs of tidal disturbances or ongoing mergers. The overall appearance suggests a massive galaxy that is likely quiescent with a moderate rate of star formation.
