The galaxy presents as a spiral type, viewed at an oblique angle. It appears relatively smooth in overall structure, with a prominent central bulge that exhibits a yellowish hue, suggesting a population of older stars. Faint spiral arms are visible extending from the bulge, displaying a bluer color, indicative of ongoing star formation. The galaxy does not show any obvious signs of major disturbances or a significant merger event. The galaxy appears to be generally well-defined and moderately luminous.
