The galaxy presents a largely smooth, elliptical morphology. There is little evidence of spiral arm structure or significant dust lanes. The central bulge appears prominent and relatively bright, displaying a yellow hue. A fainter, more diffuse halo surrounds the bulge, gradually fading into the background sky. There is no strong evidence of ongoing major merging events, though the possibility of minor disturbances cannot be entirely ruled out based on the image alone. The overall shape is closer to round than cigar-shaped. The galaxy's color suggests a population of older stars, with less active star formation.
