This galaxy appears to be a spiral galaxy, although the spiral arms are not sharply defined. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. The disk component shows hints of bluer regions, potentially indicating ongoing star formation. The galaxy has an overall elongated shape, more elliptical than circular. There is a possible merging event or tidal disturbance visible, seen as asymmetrical extensions of the galaxy's light. The overall color is shifted towards the red end of the spectrum, which is consistent with its estimated distance.
