The galaxy appears as an elongated, disk-like structure with a smooth, featureless morphology. Its color gradient suggests a higher concentration of younger, bluer stars toward the central region, transitioning to redder hues at the edges, potentially indicating an older stellar population in the outer regions. The overall shape is cigar-like, potentially an indication that it is an elliptical galaxy. There is no evidence of a recent major merger or strong tidal disturbances. The overall structure suggests a relatively evolved system.
