The galaxy presents a largely smooth morphology, with a notable central bulge. The light distribution suggests a more elliptical, rather than spiral, structure. The galaxy exhibits an intermediate roundness, appearing neither perfectly spherical nor highly elongated. There are no obvious signs of major disturbances or ongoing merging events, though subtle irregularities might suggest minor past interactions. There appears to be some bluer star formation regions primarily on the edges of the galaxy, with the core exhibiting a yellowish-red hue. The galaxy displays a moderately compact size.
