The galaxy presents as a disk galaxy, viewed nearly edge-on. A central bulge is weakly visible, exhibiting a reddish hue. The disk itself displays a mottled appearance, suggesting the presence of dust lanes and star-forming regions, primarily appearing green with hints of red. There seems to be an area of ongoing star formation within the galaxy, perhaps caused by a recent merging event. There is very weak tidal disturbance around the galaxy, but it is not strong evidence for a merger. The galaxy's light distribution appears to be fairly concentrated towards the center, indicating a possible classification as an intermediate to early-type spiral. There is no sign of a strong active galactic nucleus or a strong bar structure.
