The observed galaxy appears to be a spiral galaxy, with a dominant disk structure. The galaxy exhibits fairly well-defined spiral arms, which appear somewhat tightly wound. There is evidence of a bar-like structure bisecting the central bulge. The central bulge appears moderate in size, and exhibits a yellowish-white color indicative of older stellar populations. The spiral arms appear bluer, suggesting the presence of ongoing star formation. The galaxy disk is not perfectly edge-on, offering a good view of the spiral structure. There appears to be no obvious major merger event affecting the overall morphology, although some minor irregularities may be present in the spiral arm structure. Dust lanes are subtly visible within the spiral arms, particularly along the inner edges.
