The galaxy appears to be an edge-on spiral galaxy. A central bulge is visible, exhibiting a concentrated luminosity gradient. The disk component appears relatively smooth, lacking significant visible spiral arm structures. The disk has a flattened morphology, approximately 2.5 kpc in radius. The color of the central bulge is notably redder than the disk, suggesting an older stellar population and/or higher dust content. The disk exhibits bluer hues, indicative of younger stars and ongoing star formation, the rate of which appears to be relatively low. There are no obvious signs of recent major merger events or significant tidal distortions based on the image. The galaxy's overall appearance suggests a relatively quiescent, possibly evolved spiral galaxy.
