The object presents as a relatively compact galaxy with an overall blue hue, indicating the presence of younger, hotter stars and potential ongoing star formation. The central region exhibits high surface brightness, suggesting a dense stellar population or active galactic nucleus. The galaxy appears generally smooth in texture with no significant spiral arm structure or prominent dust lanes visible, potentially making it an elliptical galaxy. There appears to be a small hint of a disturbance along the outer rim of the galaxy. The image shows a slight asymmetry in its overall shape and there is a slight gradient change near the very center. While appearing largely undisturbed, a minor interaction or merger event cannot be entirely ruled out.
