The galaxy presents as a spiral type, with a noticeably tilted orientation relative to our line of sight, displaying a near edge-on profile. A central bulge is present, exhibiting a moderate concentration of light. The galactic disk shows evidence of spiral arm structure. Some of these arms appear tightly wound.

The blue hue suggests the presence of relatively young, hot stars, indicating ongoing star formation. Additionally, the overall morphology appears relatively undisturbed, with no obvious signs of a major merger event. A slight asymmetry is noted in the disk, hinting at a potential minor interaction or internal disturbance. Faint, diffuse outer regions are observed extending from the central structure.
