The galaxy exhibits a prominent disk structure, oriented roughly face-on relative to our line of sight. Evident spiral arms emanate from a central bulge, displaying a grand design spiral structure. The arms are somewhat tightly wound near the core and gradually loosen towards the outer regions of the disk. Two dominant spiral arms are visible. The central bulge appears relatively moderate in size, contributing significantly to the galaxy's overall luminosity. Patches of bluer hues interspersed along the spiral arms suggest regions of recent or ongoing star formation, while the bulge appears yellower/redder in color suggesting an older stellar population. There are no readily apparent signs of major interactions or mergers. Faint dust lanes can be traced along some of the inner spiral arm segments.
