The galaxy presents as a moderately luminous, elliptical structure, appearing generally smooth in texture. Its morphology is primarily spheroid with minimal disk-like features discernible. The colour profile suggests a population of older stars, with a central bulge exhibiting a yellowish-orange hue, potentially indicating a concentration of evolved stellar populations. Some blue light can be seen at the edges. The outer regions are less defined but show a slight elongation, resembling a cigar shape, and may indicate tidal interaction or that we are seeing a rotating elliptical galaxy. There are no obvious signs of ongoing major mergers or significant disturbances in its morphology, but subtle irregularities might suggest minor past interactions. Overall, the galaxy appears to be a relatively undisturbed elliptical galaxy with a substantial stellar mass and a moderate rate of star formation.
