The galaxy appears to be a relatively smooth, elliptical-like structure with a bright central bulge. Its overall shape is elongated, approaching a cigar-like morphology. There is little evidence of spiral arms or a distinct disk. The galaxy exhibits a color gradient, transitioning from a bluer hue in the outer regions to a more yellowish-white core. The outer regions have a slightly mottled appearance which might indicate recent, low levels of star formation activity, while the central bulge has a more uniform and aged stellar population. There is no obvious sign of major mergers or significant tidal disturbances, with only minor disturbances possible in the outskirts.
