The subject galaxy appears as a relatively faint, elongated spiral, oriented approximately horizontally in the image frame. The central bulge is compact and exhibits a yellowish-white hue, suggesting an older stellar population. Faint spiral arms extend outwards, showing a bluer color, potentially indicating ongoing star formation. The arms are somewhat diffuse and lack well-defined structures, lending the galaxy a slightly flocculent appearance. There is a hint of dust lanes running along the spiral arms, although these are not prominent. Overall, the galaxy exhibits a moderate redshift, indicating it is a relatively distant object. The angular size suggests the galaxy is a moderate sized spiral galaxy. Given the overall morphology and color gradients, this galaxy likely has a moderate star formation rate. There is also a low chance that this galaxy is undergoing a merger based on the morphology.
