The galaxy presents as a centrally concentrated object with a generally smooth, elliptical morphology. It exhibits a high degree of roundness. There is no discernable disk structure. No signs of a major ongoing merger event are visible, although a very subtle asymmetry on one side may indicate a minor disturbance or interaction. The galaxy appears to be relatively red in color, suggesting a population of older stars. Given the observed color and smooth morphology, this object is likely an elliptical galaxy with low star formation activity.
