The galaxy appears as a relatively small, elliptical object with a smooth, almost featureless morphology. It is dominated by light in the redder wavelengths, indicating an older stellar population with little ongoing star formation. The galaxy exhibits a high degree of roundness, with no significant distortions or tidal features apparent, except for a slight elongation. There is a slight green hue toward the center, which could be emission lines due to recent star formation or an active galactic nucleus. However, the overall smooth nature of the galaxy suggests that if an AGN is present, its contribution is small, and star formation is relatively suppressed. The light appears mostly contained within the galaxy.
