The galaxy appears as a moderately bright, elliptical-shaped object. It exhibits a generally smooth morphology, lacking significant features like prominent spiral arms or dust lanes. There may be slight hints of a disk but it mostly presents as smooth and rounded. The color distribution indicates a predominantly older stellar population, evidenced by the yellowish hue concentrated towards the center, suggesting a relatively low rate of ongoing star formation. There are no signs of major disturbances or ongoing mergers, however there may be minor disturbances. The galaxy shows a gradual decrease in luminosity from its core outwards.
