The galaxy presents as a spiral type, observed at an approximately face-on orientation. Prominent spiral arm structures are visible extending from the central region. The winding of the spiral arms appears relatively tight. There is a moderate, centrally located bulge. The disk component displays a mottled texture indicative of active star formation regions. The galaxy exhibits a blue-ish hue within the spiral arms, likely due to the presence of young, hot stars, while the bulge appears more yellow. The galaxy appears relatively isolated with no obvious signs of significant tidal disturbances or ongoing major merging events.
