This galaxy exhibits a morphology that suggests it is undergoing or has undergone a merger event. The central region is relatively smooth and concentrated, displaying a yellowish hue indicative of an older stellar population. Extending from this central region, there appears to be a prominent tidal tail-like structure, characterized by a bluer color, suggestive of more recent star formation. The overall shape of the galaxy is elongated, leaning toward a cigar shape, further supporting the likelihood of an interaction. There is some indication of disturbance of the primary galactic disc. The estimated size of the galaxy is approximately 4.7 kpc, and the redshift places it at a distance where detailed morphological features are challenging to resolve, but the observed colors and disturbed morphology suggest ongoing or recent star formation activity.
