The galaxy presents as a primarily smooth, elliptical structure. Its core exhibits a high degree of brightness, suggesting a concentrated central region. Moving outward, the intensity of light gradually decreases from the core. A subtle disk-like feature is suspected, showing a minor degree of flatness rather than a perfectly spherical shape. The color profile appears generally uniform across the galaxy, with slight variations in hue; bluer tints may indicate areas of ongoing star formation, whilst redder regions may correlate to old stellar populations. No major disturbances such as tidal tails or prominent dust lanes are observed in this image, suggesting a relatively quiescent state.
