The galaxy presents a generally smooth, elliptical morphology. A concentrated central bulge region is visible with a redder hue, suggesting an older stellar population. The galaxy exhibits a relatively high degree of roundness, with only slight elongation. The surrounding halo appears more diffuse and exhibits a bluer color, potentially indicating regions of more recent star formation, though at a low rate overall. There are no obvious signs of major mergers or significant tidal disturbances, although a subtle asymmetry suggests the possibility of a minor interaction in its past.
