The galaxy presents as a somewhat elliptical structure with a concentrated central bulge. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. Surrounding the central region, the galactic disk displays a smoother, less defined structure compared to spiral galaxies. The color transitions from yellowish-white near the center to a faint bluish tint towards the outer edges, possibly indicating younger stellar populations or ongoing star formation within the disk, although at a low rate. There is no clear evidence of distinct spiral arms or significant dust lanes, lending to its classification as likely a smooth galaxy. There is very minor asymmetry or disturbance observed in the galaxy's overall shape. The apparent roundness suggests a non-edge-on orientation relative to our line of sight.
