The galaxy presents a largely featureless, smooth morphology. Its shape appears generally elliptical, though not perfectly spherical, with a slight elongation. The light profile is centrally concentrated with a gradual falloff in intensity outwards from the core, suggesting a centrally dominant stellar population. There is no apparent disk structure, spiral arms, or prominent dust lanes visible within the galaxy. The light from the galaxy is slightly more luminous in the redder bands than the bluer bands. No obvious signs of tidal disturbances, merging activity, or active galactic nucleus are detected.
