The galaxy appears as a centrally concentrated object with a relatively smooth morphology. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. A fainter, more diffuse halo surrounds the central region, suggesting a gradual decrease in stellar density with increasing radius. There is evidence of possible tidal interaction or some other kind of merger on the bottom of the galaxy, with a faint blue region visible. Overall, the galaxy's light profile is well-defined.
