The galaxy presents as a spiral galaxy, observed at a near-edge-on angle. A central bulge appears prominent and moderately bright, displaying a yellowish hue, indicative of an older stellar population. The spiral arms are tightly wound and relatively ill-defined, suggesting a flocculent structure rather than grand design spirals. These arms exhibit a bluer color, implying the presence of younger, hotter stars and ongoing star formation. The dust lanes within the spiral arms are not clearly resolved but are likely present, contributing to the slightly mottled appearance of the disk. No significant signs of tidal disturbances or a recent major merger are immediately apparent, though minor interactions cannot be ruled out from this image alone. The overall morphology suggests a relatively undisturbed spiral galaxy with a moderate bulge size.
