This galaxy presents as a smooth, elliptical-like structure. It exhibits a bright, concentrated central bulge with a color index suggesting an older stellar population. The surrounding galactic halo appears more diffuse and subtly bluer in hue, hinting at the presence of some younger stars or ongoing, albeit relatively low, star formation. The galaxy is moderately elongated, but appears largely undisturbed, lacking any obvious signs of a major merger or significant tidal interactions. Some slight morphological irregularity might be present, but the overall structure is well-defined and relatively uniform.
