The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The light distribution is predominantly yellowish, indicating an older stellar population, though a slight gradient towards redder hues in the outermost regions is visible. The shape is moderately elliptical, not perfectly spherical, but also lacking any pronounced elongation. There is no apparent disk structure, spiral arms, or strong dust lanes visible. The overall appearance suggests a galaxy that is relatively undisturbed, showing no signs of ongoing major mergers or significant tidal interactions. The galaxy exhibits a high degree of smoothness, with no clear evidence of clumpy star-forming regions.
