The galaxy presents an overall elongated morphology, appearing roughly cigar-shaped. Its light distribution indicates a generally smooth structure, although there are subtle variations in color and intensity. The central region of the galaxy exhibits a brighter, somewhat concentrated area of bluish-white light, suggesting a region of active star formation or a dense stellar population. Towards one end of the galaxy, there is a noticeable shift in color towards a yellower or reddish hue, which could indicate an older stellar population or the presence of dust obscuring the bluer light from younger stars. There is visual evidence of a disturbance on one side of the galaxy with tidal tails, which might be the result of a recent or ongoing merger with another galaxy. Further spectroscopic and photometric analyses would be needed to confirm the exact nature of these features and fully characterize the galaxy's composition, dynamics, and evolutionary history.
