The galaxy presents an elongated, disk-like morphology, viewed at a near edge-on orientation. A central bulge is observed, exhibiting a yellowish-white hue, potentially indicative of an older stellar population. The galactic disk appears bluish, suggestive of ongoing star formation activity. Patches of slightly enhanced blue luminosity are scattered within the disk, possibly indicating regions of active star forming nebulae. There may be evidence of tidal disturbances suggesting a recent or ongoing interaction with another galaxy.
