The galaxy presents as a spiral type, exhibiting a prominent disk structure. The spiral arms are well-defined, with a relatively open morphology, suggesting a later type spiral. The galaxy's arms appear somewhat flocculent, though they generally trace a consistent winding pattern from the central bulge region. A bar feature is potentially present within the central bulge. The bulge itself appears moderately sized. There is some observed asymmetry present which may suggest minor tidal disturbance or interaction.

Color gradients are observed across the galaxy, with a yellowish hue dominating the central bulge, transitioning to bluer tones in the outer spiral arms. This implies older stellar populations concentrated in the bulge with more recent star formation occurring in the arms. There are a small number of discrete bright regions within the spiral arms, likely indicating areas of active star formation. Overall, the galaxy presents a classic spiral morphology, with features suggesting ongoing stellar evolution and potential interactions.
