The galaxy presents a generally smooth morphology, appearing as an elongated spheroid. The color gradient suggests a concentration of older stellar populations towards the central bulge, exhibiting a yellowish-orange hue. The outer regions of the galaxy show bluer tints, hinting at the presence of younger stars, possibly within a disk structure. The overall shape suggests a possible elliptical galaxy or a lenticular galaxy viewed edge-on. There is little evidence of ongoing major mergers or significant tidal disturbances. Minor asymmetries and irregularities are subtly apparent, potentially caused by minor interactions.
