The galaxy presents as a relatively smooth, elliptical morphology, with minimal discernible features indicative of spiral arms or a distinct disk. It appears somewhat flattened in shape. The color distribution suggests a dominant population of older stars, with a central region exhibiting a more concentrated luminosity. There appears to be only a very small amount of recent star formation occurring. There's no indication of ongoing major mergers or significant tidal disturbances affecting its overall structure.
