The galaxy presents as a slightly elongated, diffuse structure. The central region exhibits a high degree of luminosity, appearing smooth and concentrated, suggesting a bulge. Moving outward from the core, there is a transition to a less defined region. There is a slightly asymmetric extension or tidal feature to the right of the galaxy in the image. The color profile indicates a dominance of redder wavelengths overall with bluer knots appearing in the fainter regions, hinting at possible regions of recent star formation. There appears to be minor gravitational disturbances, possibly the result of an ongoing merger with a smaller galactic object or a close encounter with another galaxy.
