The galaxy appears to be relatively small and compact. It exhibits a bright, concentrated central region. There is a notable asymmetry, with some disturbances visible within the overall structure. A faint disk feature can be discerned, with some regions appearing somewhat warped or irregular. There are hints of tidal tails or debris, which suggests past or ongoing interactions with another galaxy. The color distribution indicates varying stellar populations, with the central bulge exhibiting a bluer hue and outer regions displaying a range of colors. The presence of redder regions suggests the existence of dust lanes or regions of ongoing star formation. Overall, the galaxy appears to be in a state of dynamic change or possible merger activity.
