The galaxy presents as a spiral type, oriented at a slight angle relative to our line of sight. Distinct spiral arms are visible, though somewhat tightly wound. The central bulge is moderate in size and exhibits a yellowish hue, possibly indicating an older stellar population. The spiral arms appear bluer, suggesting ongoing star formation. Two main arms are visible which extend outwards from the central bulge. The spiral arms are relatively well defined and somewhat patchy, possibly due to the clumpy nature of star-forming regions within the arms. There is no apparent major disturbance or merger event ongoing. The galaxy does not appear to be significantly edge-on. A slight bar structure is present within the central region. The overall morphology appears well-formed.
