The galaxy presents as an elongated, disk-like structure, viewed at an oblique angle. The central region exhibits a yellowish-white hue, indicative of an older stellar population. Moving outwards, the galaxy displays bluish tones, particularly noticeable at the edges of the disk. These areas may indicate regions of ongoing star formation. The overall structure appears relatively smooth with a moderate concentration of light towards the center. There is a suggestion of some minor disturbance in the disk, which may indicate a past or ongoing interaction. There may be signs of past merger activity but overall the galaxy does not appear to be currently undergoing a major merger event. The galaxy appears to be moderately massive and exhibits a moderate amount of star formation.
