The galaxy presents as a spiral type, observed at a slight angle relative to face-on. It exhibits a bright, concentrated central bulge, appearing yellow-white in color, suggesting an older stellar population. A bar feature is faintly visible, bisecting the bulge along its major axis. The spiral arms are well-defined, though tightly wound, displaying a somewhat flocculent morphology with localized knots of blue light indicative of active star formation regions. The disk component appears relatively flattened. Dust lanes are subtly apparent along the inner edges of the spiral arms, contributing to a mottled appearance. No significant tidal features or signs of a major merger are immediately discernible. The overall color gradient suggests a transition from an older, redder population in the bulge to a younger, bluer population in the arms.
