The galaxy presents as a relatively smooth, elliptical morphology. Its central bulge exhibits a bright, concentrated luminosity, indicative of a high stellar density. The galaxy's overall color profile appears slightly redder, suggesting a population of older stars and a reduced rate of ongoing star formation. There are hints of a disk structure, though any spiral arms, if present, are faint and tightly wound, or possibly absent altogether. The galaxy's shape approximates a flattened spheroid with axial asymmetry, and shows no obvious signs of tidal disturbances or ongoing mergers with other galaxies.
