The galaxy presents a morphology that leans towards being smooth, exhibiting a degree of circularity, though some deviation from a perfect circle is observed. It shows a distinct central bulge, the brightest and most concentrated region of the galaxy, which graduates into a less-defined and somewhat elongated outer halo.

Color gradients are apparent, with the central bulge exhibiting a yellowish hue, potentially indicative of an older stellar population. The outer regions show hints of bluer colors, which could be due to the presence of younger stars or ongoing star formation.

There is a suggestion of faint, diffuse features that might be indicative of minor disturbances, possibly from interactions, although the galaxy's overall structure remains largely undisturbed. The luminosity profile appears relatively smooth.
