The galaxy presents a morphology indicative of a spiral or disk-shaped galaxy, observed at an oblique angle to our line of sight. A notable feature is the presence of a prominent central bulge that displays a smooth, concentrated light profile.

The galaxy exhibits a distinct color gradient. The central bulge and parts of the disk show a yellowish or reddish hue, potentially indicating an older stellar population. This contrasts with areas of the disk that show a hint of bluer light, possibly signaling regions of ongoing star formation.

There is a potential interaction or disturbance that appears to be present in the galaxy. The disk appears somewhat irregular or asymmetric. The galaxy's morphology suggests that this may be a potential merger, with tidal tails possibly visible.
