This galaxy presents as an irregular system. A significant portion of the light appears concentrated within a bright, relatively circular central region. This core exhibits a smooth, homogenous texture. Extending away from the main body is a fainter, more diffuse tidal feature which might be caused by merging activity. This tail has a bluer hue, suggesting the presence of younger stellar populations relative to the central concentration. The overall shape deviates significantly from a standard elliptical or spiral morphology. There is evidence for ongoing or recent gravitational interaction, which is causing the irregularity of the system.
