The galaxy presents as an elongated structure with a moderately inclined disk. The disk component displays evidence of internal structure, exhibiting a color gradient. The central region exhibits a yellow-orange hue, potentially indicative of an older stellar population. Towards one end of the galaxy, a distinct greenish-blue region suggests more active star formation. Overall, the galaxy appears somewhat disturbed, lacking a perfectly smooth or symmetric structure. There is potential evidence of tidal features, but it is difficult to tell, without further investigation. The galaxy does not show clear evidence of a major merger, however minor disturbances are likely.
