The galaxy presents as a singular, relatively smooth, and concentrated entity. The overall morphology appears elliptical, with a high degree of central concentration. The light distribution is fairly symmetrical with a smooth profile, transitioning gradually from the central core outwards. The color suggests a population of older stars, with a redder hue dominating its overall appearance. There is no apparent presence of spiral arms or a defined disk structure. The galaxy does not appear to be undergoing any major merging events or tidal disturbances. The apparent size is small, indicating that it is a distant galaxy.
