The galaxy exhibits a generally smooth morphology, with a notable central bulge. The overall shape appears elliptical, deviating slightly from perfect circularity, tending towards an in-between form. There is some indication of disk-like features or spiral arms, though these are subtle and not well-defined.  The color gradient suggests a mixed stellar population, with a concentration of older, redder stars in the bulge region.  There is a possibility of minor disturbances in the galaxy's structure, perhaps suggestive of a past interaction or minor merger.
