The galaxy presents a generally smooth, elliptical morphology. Its core exhibits a bright, concentrated luminosity, shifting towards longer wavelengths, suggestive of an older stellar population. Fainter, more diffuse light extends outwards from the core, but lacks defined spiral arm structures or distinct features. There is a slight elongation, but overall, the galaxy presents a nearly circular appearance on the sky. There is no clear indication of ongoing major mergers or significant tidal disturbances, although very subtle irregularities might be present. Based on the color profile, star formation activity appears to be subdued.
