The galaxy presents as a relatively smooth, elliptical-like structure. It displays a centrally concentrated bulge that gradually diffuses outwards into a less defined halo. There are no prominent spiral arms or bar features visible. Color gradients suggest that the central bulge is likely populated by older stars, appearing slightly redder. The outer regions exhibit a bluer hue, possibly indicative of younger stellar populations or ongoing, albeit low, star formation. No major disturbances or signs of ongoing merger activity are clearly observed, although there is a hint of a minor asymmetry in the outer halo. The galaxy exhibits an overall regular shape, appearing mostly rounded with a slight deviation toward an elongated form. Its size is small to moderate relative to other galaxies in the field of view.
