The galaxy presents as a relatively smooth, elliptical-like structure with a highly concentrated central bulge. It exhibits a generally featureless morphology, lacking any obvious spiral arms, dust lanes, or distinct star-forming regions visible at this resolution. The galaxy appears slightly flattened, transitioning from a circular core to a more elongated outer halo. The color profile suggests a population of older stars, based on its redder hue, with very little blue light indicating the presence of young, hot stars or recent star formation. There are only minor disturbances suggesting this galaxy is not currently undergoing a major merger.
