The galaxy presents as a generally elliptical form, appearing more rounded than elongated. A bright, concentrated central bulge dominates the galaxy's light profile, suggesting a significant population of older stars. The luminosity decreases gradually from the core outward.

The overall color is yellowish-white, indicative of a relatively quiescent stellar population with minimal ongoing star formation. There's a hint of bluer light at the extreme edges of the disk, perhaps suggesting the presence of younger stars.

No distinct spiral arm structures or prominent dust lanes are discernible. Faint tidal features are not obvious, nor are signs of any major ongoing or recent mergers. The galaxy appears relatively undisturbed and evolved, exhibiting a smooth, symmetrical morphology.
