The galaxy appears to be a spiral galaxy, presenting a near edge-on orientation with a high inclination to our line of sight. A prominent central bulge exhibits a smooth, concentrated brightness profile, surrounded by a flattened disk component. Faint, tightly wound spiral arms emanate from the central region, displaying a blue hue indicative of recent or ongoing star formation activity. No obvious signs of a strong bar structure are apparent. The spiral arms are somewhat difficult to discern and seem to fade into the surrounding space. There does not seem to be much disruption to the main body of the galaxy.
