The galaxy exhibits an elliptical morphology. The light distribution appears somewhat uniform, with a central concentration of luminosity. There is no clearly discernible disk structure. A fraction of the galaxy appears more smooth, while a small portion shows some disturbed features. This may be indicative of a minor interaction or recent merger event. The color distribution suggests a population of older stars, with a reddening towards one edge. There may be a small amount of dust obscuring some regions, potentially contributing to the observed redder colors.
