The galaxy presents a disturbed morphology, possibly indicative of a recent or ongoing interaction. It exhibits an elongated shape with a primary central region of increased luminosity. A secondary, less luminous extension or tidal feature is visible, emanating from the main body. Color gradients are observed, with a bluer hue concentrated in what appears to be the nucleus and portions of the extended structure. This suggests the presence of younger stellar populations and ongoing star formation in those areas. The overall structure hints at potential merging activity or a close encounter with another galaxy. The presence of a secondary disturbed feature is a strong possibility to confirm some kind of merging or gravitational interaction. There is no presence of a spiral structure, and the galaxy is of a medium size, without appearing particularly massive.
