The galaxy presents a somewhat elongated morphology. Its central region is noticeably brighter, exhibiting a yellowish-white hue, which may indicate an older stellar population. Surrounding the core, a fainter, bluish halo is visible. This suggests the presence of younger stars or ongoing star formation activity in the outer regions. There is some indication of potential tidal disturbances, which could be attributed to a possible past interaction with another galaxy. The galaxy appears relatively smooth in texture, although the faintness of the image makes it difficult to determine the presence of distinct spiral arms or other defined structures with certainty.
