The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light profile appears elliptical, tending towards an intermediate ellipticity rather than being perfectly circular. Some asymmetry is visible, possibly indicating minor disturbances in the galaxy's structure. There is no strong evidence of spiral arms or a prominent disk. The central region appears to be a yellowish color, possibly indicating an older stellar population, with bluer colors towards the edge of the galaxy. Overall, the galaxy appears to be relatively isolated, showing no strong signs of recent or ongoing major merger activity.
