This galaxy appears to be undergoing a significant interaction or merger. There are two distinct luminous components visible, suggesting either a close pair of galaxies or a single galaxy with a strongly disturbed morphology. The primary component appears relatively smooth, with a concentrated central region and a diffuse surrounding halo. The secondary component is less distinct, with a slightly fainter and more irregular appearance. The color of both components indicates the presence of older stellar populations, with a stronger contribution from redder wavelengths, suggesting lower levels of recent star formation activity. Possible tidal features or bridges of material are subtle or obscured, but the overall morphology points towards an ongoing or recent gravitational interaction. The galaxy's general shape is more rounded than elongated, and its proximity suggests that it is relatively large in physical size.
