The galaxy appears to be a single, relatively smooth and centrally concentrated object with no obvious spiral arm structure or prominent disk features visible at this resolution. Its shape appears to be more ellipsoidal than disk-like. There is some evidence of minor disturbance, possibly a companion galaxy in close proximity, which shows some tidal disturbance. The primary body of the galaxy exhibits a color gradient, with a slightly bluer hue in the outer regions transitioning to redder tones toward the center. This could indicate ongoing or recent star formation activity in the outer parts, with an older, redder stellar population dominating the core. The overall luminosity of the galaxy appears substantial. The galaxy does not appear to be undergoing a major merger, but might be experiencing some tidal interactions.
