The galaxy appears as a centrally concentrated object with a generally smooth morphology. The central region exhibits a bright, yellow-white core that diminishes in intensity outwards. The galaxy lacks any apparent spiral arm structures or a distinct disk, suggesting a more elliptical or lenticular classification. There is a slight deviation from perfect circularity but the galaxy appears mostly circular. There is no evidence of tidal tails or major mergers, although some subtle asymmetry might indicate minor gravitational interaction or recent accretion events. The color suggests a population of older stars, with relatively little ongoing star formation.
