The galaxy presents a generally smooth, elliptical appearance, with a high degree of central concentration. It exhibits a subtle color gradient, appearing slightly bluer towards its periphery than its center. There is a hint of a flattened structure, but no distinct spiral arms or strong disk features are discernible. Minor disturbances or mergers cannot be ruled out due to some clumpy features at the galaxy's edge, and a merging event may have occurred at some point in its past. The galaxy has an intermediate degree of roundness. The galaxy's estimated size is approximately 3.5 kpc. The absolute magnitude suggests it is a relatively luminous galaxy, with a notable amount of ongoing star formation.
