The galaxy presents as an elongated spiral, viewed at a significant inclination relative to our line of sight. A bulge, somewhat brighter than the rest of the disk, is visible at the center. The disk appears to be populated with spiral arms, though they are not sharply defined, possibly due to distance or inclination effects. The overall light distribution is not uniform throughout the disk. Some areas within the disk may indicate ongoing star formation activity. The colors appear more blueish/white across the majority of the galaxy, though towards the bulge this seems to transition to more yellow. There might be a bar structure present in the center, but it is not very strong or well-defined in this image. Based on this image alone, there is no evidence of any major merger events or significant tidal disturbances.