The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated, bright central region. The core appears yellowish-white, suggesting a population of older stars. There is a gradual decrease in luminosity moving outwards from the center, with the outer regions displaying a slightly redder hue. The overall shape is moderately elongated, not perfectly spherical. There is no visible evidence of spiral arms or significant dust lanes. The general appearance suggests a galaxy that has largely ceased active star formation, with a dominant population of evolved stars. There is no clear indication of major mergers or tidal disturbances.
