The galaxy presents as a moderately luminous, disk-shaped structure oriented approximately edge-on relative to our line of sight. A central bulge is visible, exhibiting a yellowish-white hue, suggesting a population of older stars. The galactic disk appears to be relatively smooth, with some evidence of subtle, diffuse spiral arm structure detectable. The outer regions of the disk display a bluer color, possibly indicating ongoing star formation. The morphology suggests a classification somewhere between an elliptical and spiral galaxy. There is a minor asymmetrical disturbance on the left side of the disk. No evidence of a major merger is apparent in this image, but some level of minor tidal interaction cannot be excluded based on the asymmetry.
