The galaxy appears to be an elliptical type, exhibiting a smooth, relatively featureless morphology. The object's color profile suggests a population dominated by older stars, with a yellowish central bulge transitioning to slightly bluer hues in the outer regions. This potentially implies ongoing, but subdued, star formation in the disk. The galaxy is not perfectly round, displaying a subtle elongation that hints at an intermediate shape between a sphere and a flattened disk. There's no immediately obvious evidence of significant tidal disturbances or ongoing mergers, although a slight asymmetry could indicate minor gravitational interactions in the recent past. Overall, the galaxy presents as a mature, relatively quiescent system.
