The galaxy presents a predominantly smooth morphology, with an overall elliptical shape. The central region exhibits a concentrated, bright core, likely indicating a significant stellar density or possible active galactic nucleus. There's a noticeable color gradient from the center outwards, shifting from yellowish-white to a faint bluish hue in the outer regions. This suggests a difference in stellar populations, with older, redder stars concentrated towards the core and younger, bluer stars residing in the outskirts. There is a slight asymmetry, but it does not appear to be undergoing a major merging event, but subtle disturbances are not completely ruled out. No distinct spiral arms or prominent dust lanes are apparent in this image.
