The galaxy presents as a spiral type, characterized by a central bulge that transitions into a well-defined disk. Evident spiral arm structures emanate from the central region, exhibiting a relatively open morphology. The arms appear somewhat patchy and less tightly wound, suggesting ongoing star formation. The disk shows variations in color, with bluer regions indicating the presence of younger, hotter stars, interspersed with older, yellower stellar populations. The galaxy appears moderately inclined, with some obscuration potentially due to dust lanes within the disk. The overall shape is not perfectly regular, possibly indicating minor gravitational interactions or internal asymmetries. There is a subtle bar-like structure that seems to be a weak feature. There does not seem to be any sign of merging or major disturbances in the galaxy, as its structure seems well defined.
