The galaxy presents as a relatively faint, elongated object with a clear disk structure. It is observed nearly edge-on. The central bulge is not prominent, appearing quite small and only slightly brighter than the rest of the disk, which is not very luminous either. There appears to be some dust obscuration, visible as subtle dark lanes running along the length of the disk. These lanes might be impacting the light emitted from the disk. No distinct spiral arm structures or star-forming regions are immediately apparent based on the image. There are no signs of significant tidal disturbances or ongoing major merging activity. The galaxy appears to be relatively isolated and undisturbed.
