The galaxy appears as a relatively compact and bright object with a somewhat elliptical morphology. Its light distribution is dominated by a smooth, centrally concentrated bulge. There is a faint suggestion of a disk, which is a flattened, more extended structure, surrounding the central bulge. The disk component seems to be weakly defined. No spiral arms or distinct star-forming regions are visually apparent in this image, which indicates that star formation is either low or obscured by dust within the galaxy. There is no obvious sign of ongoing major or minor mergers with other galaxies; however, there is a small chance that the galaxy is undergoing a merger or a tidal event. Overall, this galaxy likely has an older stellar population. It may be characterized as a passive or quiescent galaxy.
