The galaxy presents a predominantly smooth, elliptical morphology. It appears elongated, but not highly so, displaying an intermediate roundness. There is a suggestion of a slight disturbance or feature within its structure, potentially indicating a minor interaction or internal activity. The galaxy exhibits a distinct blue hue, with a brighter central concentration and a gradual fading toward the edges. This color suggests a moderately active star formation rate within the galaxy. Overall, the galaxy appears to be a massive, relatively evolved system undergoing some degree of ongoing star formation and possibly experiencing subtle gravitational interactions.
