This galaxy appears to be undergoing a merger. Two distinct components are visible: one exhibits a yellowish-white color with a smooth, rounded morphology, while the second shows a bluer hue and a less defined, more disturbed structure. The bluer component suggests ongoing or recent star formation, possibly triggered by the interaction. The yellowish-white component likely contains an older stellar population. A faint tidal bridge may be present between the two, further indicating gravitational interaction. Overall the galaxy appears quite compact, and a moderate redshift suggests the galaxy is far away.
