The galaxy presents a largely smooth and elliptical morphology. There is an observed color gradient transitioning from a yellow-white central bulge to a redder outer halo, suggesting a radial change in stellar population. The central region appears more luminous and densely populated with older stars relative to the galactic periphery. Hints of disklike or featured morphology are visible in the outer regions, but these are relatively muted. The galaxy is not exhibiting any major signs of ongoing merger activity or significant tidal disturbances. The lack of distinct spiral arms or prominent dust lanes indicates it is likely an elliptical galaxy with relatively low levels of star formation at the epoch of observation.
