The galaxy appears to be a relatively smooth, elliptical system. Its light profile indicates a high degree of central concentration. The primary color of the galaxy is a yellowish-orange hue, suggesting an older stellar population, with only minimal ongoing star formation. The galaxy presents a rounded morphology and appears largely undisturbed, showing no signs of significant tidal interactions or recent mergers, although a very slight asymmetry is present in its light distribution. Some minor disturbances are present, suggesting that perhaps a past merger or interaction may have occurred. Overall, the galaxy presents a consistent and relatively relaxed structure.
