The galaxy appears as a diffuse, elongated object with a bluish hue. Its structure is not well-defined, but appears to be somewhat smooth, though at least one possible tidal tail appears to exist. There is a bright central concentration of light, but without a sharply defined nucleus. The galaxy exhibits some irregular features, suggesting potential gravitational interactions or internal disturbances. There is some asymmetry in the light distribution. There are some fainter regions and extended structure, which could indicate star formation regions or tidal debris, respectively. Overall, the galaxy presents an interesting morphology suggestive of a system undergoing some sort of interaction or disruption.
