The galaxy presents as an elliptical morphology, appearing largely smooth and concentrated towards the center. The light profile exhibits a radial gradient, with the core exhibiting a bright, yellowish hue that transitions into a fainter, reddish-orange halo. There is no discernible spiral arm structure or significant dust lane obscuration, suggesting a relatively old stellar population. The overall structure is quite symmetric and well-defined, with a generally circular appearance, with only the slightest hint of elongation. There are no obvious signs of major mergers or tidal disturbances in the immediate vicinity of the galaxy.
