The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. There is a noticeable color gradient, transitioning from a yellowish-white core to a more reddish outer halo. No distinct spiral arms or significant dust lanes are apparent. The galaxy exhibits a high degree of symmetry, with only subtle deviations from perfect ellipticity. There are no indications of ongoing major mergers or strong tidal disturbances, though a very slight asymmetry might suggest minor interaction or past accretion events. The overall appearance suggests a relatively evolved system dominated by an older stellar population with a low rate of current star formation.
