The galaxy presents as an edge-on spiral or lenticular galaxy with a high degree of inclination relative to our line of sight. A prominent central bulge dominates the morphology, exhibiting a yellowish hue, indicative of an older stellar population. The disk component, while less distinct, shows a faint, bluish tinge, particularly noticeable in the upper region of the galaxy. There is a slight indication of dust lanes within the disk, obscuring the light from stars behind them, but they do not appear to be significant. The overall structure is relatively smooth, with no strong evidence of spiral arm structure in this image. The shape is elongated, demonstrating a length more than twice its width. The light tapers off gradually from the bright central bulge towards the edges of the galactic disk, which suggests that the disk is truncated with a relatively small radius.
