The observed galaxy presents a distinct disk morphology. The galaxy's disk is oriented approximately edge-on relative to our line of sight. There's a prominent central bulge, appearing bright and relatively smooth in texture. Traces of spiral arm structure are visible extending from the central bulge, though these are somewhat obscured by the edge-on perspective. The dust lanes within the disk appear dark, attenuating the light from the stars behind. The galaxy exhibits a subtle blueish hue in some regions of the disk, which might indicate areas of recent star formation. A faint structure appears close to the galaxy. Overall, the galaxy seems to be a relatively well-defined spiral galaxy, potentially undergoing some minor gravitational interaction.
