The galaxy presents an elliptical morphology, characterized by a smooth, diffuse light distribution without prominent spiral arms or a well-defined disk. The central region appears brighter and more concentrated, suggesting a bulge. The galaxy exhibits a moderate flattening, with an ellipticity that is neither perfectly circular nor highly elongated. There are no distinct tidal features or signs of recent mergers, implying a relatively undisturbed evolutionary history. The color gradient seems fairly uniform across the galaxy, with a slightly redder hue toward the core, indicative of an older stellar population and diminished star formation activity. Overall, the galaxy appears as a mature elliptical system with a smooth stellar profile and quiescent star formation.
