This galaxy appears to be a spiral galaxy, viewed almost perfectly edge-on. A prominent bulge is evident, exhibiting a rounded morphology. The disk is quite thin and elongated, displaying a slight warp or unevenness along its length. Faint, diffuse dust lanes are possibly present within the disk structure, absorbing light and creating subtle dark patches. Star formation seems to be occurring at a moderate rate. The light is shifted towards the redder end of the spectrum which suggests that it is at a significant distance from our own. No signs of major mergers or tidal disturbances are obvious.
