The galaxy presents as a somewhat faint, elongated structure. There is a disk like component which appears slightly edge-on from our vantage point. A faint central bulge is present but appears to be small. There are hints of spiral arm structure, but they are not well-defined, possibly due to the viewing angle. The galaxy exhibits a blue hue overall, which may be indicative of recent or ongoing star formation within the disk. There appears to be some patchy morphology throughout the disk, potentially related to dust lanes or regions of enhanced star formation. The galaxy doesn’t appear to be undergoing any major merging events, but there is a possibility of some minor disturbances.
