The galaxy presents as a dominant, elliptical morphology. A smooth, centralized bulge is prominent with a yellow-orange hue, suggesting an older stellar population. Faint and diffuse light surrounds the central bulge, exhibiting a gradual fading outwards. The overall structure appears largely undisturbed, with no obvious signs of tidal features or ongoing major mergers, however a very faint hint of a blue tinge can be seen on the edge of the galaxy suggesting a possibility of minimal star formation. The galaxy's form is generally consistent with a high degree of rotational symmetry, showing a mildly elongated profile.
