The galaxy presents as a disk galaxy, viewed nearly edge-on from our vantage point. A distinct, though subtle, bulge is observed at the center. The bulge appears relatively smooth and featureless. The disk itself exhibits a higher degree of heterogeneity in color and luminosity. There are notable blue regions particularly toward one end of the disk, likely indicating areas of recent or ongoing star formation. Darker dust lanes are subtle, but appear present along the disk, obscuring the light emitted from regions within the plane of the galaxy. Overall, the galaxy exhibits a morphology consistent with a relatively quiescent system, but with some evidence of ongoing star formation activity.
