The galaxy presents as a flattened, elongated object with a distinct cigar shape. Its structure appears relatively smooth overall, but there is a suggestion of disk-like morphology. The color gradient shifts from a bluer hue toward the center of the disk, indicating potential recent star formation or a younger stellar population residing there, to a redder hue at the galaxy's extremities. The light distribution suggests a central bulge that extends into a disk, with no strong evidence of spiral arms. The galaxy does not obviously present any signs of any major ongoing merger events, though there is some indication of a possible tidal tail.
