The galaxy presents as a disk galaxy viewed at a near edge-on inclination. A central bulge is visible, appearing roughly spherical and displaying a concentrated luminosity gradient. The disk component exhibits a flattened morphology, with a somewhat irregular distribution of light. There appears to be a slight disturbance, possibly a minor interaction or tidal feature, along one edge of the disk. Light from the disk has a bluer hue than the central bulge, which may indicate ongoing star formation within the disk. The galaxy shows no strong evidence of a major merger, although some asymmetries are observed within the disk structure. Overall, the galaxy appears to be a disk galaxy with a relatively high inclination, exhibiting possible signs of interaction and ongoing star formation.
