The galaxy presents as a faint, irregularly shaped object with a slightly elongated morphology. The overall color is bluish, suggesting the presence of relatively young, hot stars. There is a noticeable lack of a defined central bulge or spiral arm structure. The light distribution appears uneven, with some areas exhibiting brighter, concentrated patches of emission. The galaxy does not appear to be a pure elliptical, but instead shows hints of disk-like features, though the disk is significantly disturbed. There is a possibility of tidal features indicating an interaction or merger, as indicated by the irregular shape. Based on its color and morphology, star formation appears to be ongoing, but not at an extreme rate. The galaxy exhibits some degree of smoothness, with some regions appearing diffuse and unstructured. There's no evidence of a dominant active galactic nucleus.
