The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. The core exhibits a bright, yellowish hue, suggesting a concentration of older stellar populations. Moving outward from the core, the color transitions into a bluer halo, possibly indicating the presence of younger stars or ongoing star formation in the outer regions. The overall shape of the galaxy is somewhat elongated, with a slight cigar-like appearance. No distinct spiral arms or strong dust lanes are readily apparent. There are no obvious signs of major mergers or significant tidal disturbances affecting the galaxy's structure. Minor irregularities may exist in the outer regions, but these do not dominate the galaxy's overall morphology.
