The galaxy presents a clear disk-like structure, observed at a significant inclination, placing it near edge-on from our perspective. A central bulge is apparent, exhibiting a yellowish-orange hue, possibly indicative of an older stellar population. Extending outwards from the bulge is the galactic disk, displaying a bluer tint, suggesting ongoing star formation. The disk is not perfectly smooth, showing some irregularities and hints of spiral arm structures, though these are somewhat indistinct. There is a suggestion of minor tidal disturbance or interaction, apparent as a faint extension or distortion on one side of the galaxy, possibly indicating a past or ongoing minor merger event. Overall, the galaxy appears to be a spiral galaxy undergoing active, but not extreme, star formation.
