The observed galaxy presents as a disk galaxy, oriented edge-on from our line of sight. The central bulge appears relatively prominent and has a boxy shape, with a moderate amount of light concentrated towards the center. There is evidence of a flattened disk extending outwards from the bulge, appearing relatively smooth with a lack of distinct spiral arm structures. Based on the color profile, there may be regions of ongoing star formation, however they do not dominate. The galaxy appears relatively isolated, without evidence of a major ongoing merger or significant tidal distortions. The galaxy's morphology suggests that it has been evolving relatively undisturbed over a significant period.
