The galaxy appears as a relatively smooth, centrally concentrated object, likely an elliptical galaxy or a lenticular galaxy seen at a slight angle. Its light is dominated by a slightly redder hue, suggesting an older stellar population. It exhibits a generally elliptical morphology, with a high degree of roundness. There is no obvious sign of spiral arms, a bar, or any major disturbance, although a slight asymmetry in the outer regions suggests a possible minor interaction or past merger event. No signs of ongoing active star formation are visible, although this does not preclude a low-level of star formation activity. The galaxy appears relatively isolated in the image, without any large companion galaxies in close proximity.
