The galaxy appears to be a relatively smooth, elliptical type. There is a subtle color gradient from the center outwards, with the core appearing slightly redder and transitioning to bluer hues further from the center, suggesting older stellar populations in the core and younger populations in the outer regions. The galaxy presents with a slightly elongated shape, but largely rounded. There are no strong signs of prominent spiral arms or a distinct disk structure. The light is centrally concentrated, with a gradual decrease in brightness towards the outer edges. There does not seem to be an active galactic nucleus visible in this image, although this could be due to resolution limitations. The galaxy does not appear to be undergoing a major merger or strong tidal interaction with another galaxy. There may be evidence of a minor disturbance or interaction, but this is not conclusive from this image alone.
