The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a flattened, elliptical morphology. The radial color gradient suggests a potential difference in stellar populations between the core and outer regions, with bluer colors, indicating recent star formation, possibly more prevalent in the outer regions. The overall structure lacks prominent spiral arms or other distinct features, suggesting it is likely an early-type galaxy. There is minimal evidence of significant tidal disturbances or ongoing major merger activity. Faint asymmetry or minor irregularities hint at possible past interactions or minor accretion events. The galaxy has a red shift of roughly 0.175. Given the galaxy's size and morphology, it is likely a sizable object with a significant mass.
