The galaxy presents as a disk galaxy, observed edge-on relative to our line of sight. It exhibits a prominent central bulge which is not boxy, appearing somewhat rounded. The disk is relatively smooth in appearance, with no immediately obvious dust lanes or spiral arm structures visible, potentially due to the edge-on orientation. The galaxy appears to have a moderately low star formation rate, as there are no prominent regions of intense blue light indicative of strong star formation activity. The overall light distribution appears symmetrical. There are no obvious signs of tidal disturbance or interactions with nearby galaxies, suggesting it is likely a relatively isolated system that is not undergoing any major merging events.
