The galaxy appears to be a spiral galaxy with a central bulge and a surrounding disk. The central bulge exhibits a smooth, relatively uniform luminosity profile. The disk shows some faint features, possibly spiral arm segments, though these are not sharply defined. The color suggests the presence of star formation regions within the disk. There are hints of a possible minor merger or tidal disturbance. There seems to be a faint stream of light, possibly caused by a merger event. The overall shape of the galaxy appears somewhat irregular, which could indicate gravitational interaction with another galaxy or ongoing merger activity.
