The galaxy presents as a spiral type, with a moderately sized bulge relative to the disk. The spiral arms appear distinct and well-formed, displaying a two-arm structure. The winding of these arms is intermediate, neither tightly wound nor completely open. The disk exhibits a somewhat clumpy structure, suggestive of active star formation regions within the arms. There are subtle hints of disturbances in the outer regions of the disk, indicating possible past minor interactions or accretion events. The central bulge appears relatively smooth and concentrated. The overall color profile suggests a mixture of stellar populations, with bluer regions likely corresponding to younger stars in the spiral arms, and yellower hues indicating older stellar populations within the bulge. The galaxy is not seen edge-on.
