The galaxy presents a somewhat diffuse, elliptical morphology. The central bulge exhibits a yellowish hue, suggesting a population of older, less massive stars. Moving outward from the core, the galactic disk displays a bluer color, indicative of ongoing star formation. There are only subtle signs of any spiral arm structure or distinct features, with the galaxy appearing relatively smooth in overall texture. While the galaxy appears mostly undisturbed, there is a slight asymmetry in the distribution of the bluer light in the galactic disk, hinting at a possible minor interaction or disturbance in the past.
