The galaxy presents as a relatively smooth, elliptical-like structure. Its overall morphology appears largely undisturbed, with no major signs of mergers or significant tidal interactions. The light distribution is centrally concentrated, exhibiting a bright, well-defined core that gradually diffuses outwards. The galaxy appears almost perfectly round. The color profile is predominantly yellowish-white, suggesting an older stellar population with relatively low ongoing star formation activity. There is no visible evidence of strong spiral arm structures or prominent dust lanes. The overall appearance suggests a evolved galaxy with a high degree of spheroidal symmetry.
