The galaxy presents a largely smooth, elliptical morphology. Its overall shape appears nearly circular. A bright, concentrated central bulge is observed, suggesting a high stellar density within this region. The color profile indicates a relatively even distribution of older stellar populations, potentially with some ongoing star formation, as subtle blue tints are discernible at its outermost edges. There's no apparent presence of prominent spiral arms or significant dust lanes. The galaxy does not appear to be undergoing any major merging events or experiencing significant tidal disturbances, although there is some evidence of minor disturbances in the surrounding halo of the galaxy. Overall, the galaxy seems to be relatively evolved and stable.
