The galaxy presents as a somewhat elliptical, centrally concentrated light source. It exhibits a relatively smooth morphology, lacking distinct spiral arm structures or prominent dust lanes within the resolution limits of the image. The central region appears brighter and exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Moving outwards from the center, the galaxy transitions to a more diffuse, bluish-white glow, possibly indicating the presence of younger, hotter stars. There is a subtle asymmetry, with a slight elongation observed along the major axis. No significant tidal features or signs of ongoing major mergers are discernible, though subtle disturbances cannot be entirely ruled out. The overall color profile suggests a galaxy transitioning away from active star formation, with a mixed population of older and younger stars.
