The galaxy presents a generally smooth appearance, with an overall elliptical shape. The light distribution is not uniform, showing a brighter, more concentrated region to the left, with bluer tones, suggesting a region of active star formation. To the right of the central region, a slightly elongated, redder area is visible, possibly indicating an older stellar population or significant dust extinction. There is some evidence of minor disturbance in the overall structure, possibly due to tidal interactions or an ongoing merger.
