The galaxy presents as a relatively small, faint, disk-shaped structure. The disk appears to be viewed at a near edge-on inclination. A central bulge is visible, exhibiting a concentrated, bright region with a slightly more yellowish hue, suggesting an older stellar population. The surrounding disk shows a bluer color, indicative of ongoing star formation within. Some patchy regions within the disk suggest the presence of spiral arm structures, though the image resolution limits a clear definition. The galaxy shows signs of minor disturbances. The overall morphology suggests a spiral galaxy type, though some irregularity suggests possible interactions or recent mergers.
