The galaxy presents a largely elliptical morphology, appearing generally smooth with a concentrated central bulge.  The color gradient suggests a stellar population that is older and redder in the core, becoming slightly bluer in the outer regions, which could indicate more recent, though still moderate, star formation activity in the galactic disk. There is no clear evidence of spiral arms or a distinct disk structure from this view, nor are there signs of significant tidal disturbances or ongoing major mergers, though a minor disturbance cannot be completely ruled out. Overall, the galaxy's appearance is consistent with that of an early-type galaxy undergoing a period of slow evolution.
