The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, largely featureless morphology. The color gradient suggests a reddish hue in the central regions, possibly indicative of an older stellar population concentrated towards the core. Fainter, bluer emissions appear distributed throughout the galactic disk, potentially signifying more recent star formation. The disk shows some subtle evidence of disturbance or asymmetry, such as a slight warping of the disk in the upper section. Overall, the galaxy appears to be a relatively massive system with moderate star formation activity and a predominantly smooth profile.
