The galaxy exhibits a distinct spiral morphology, characterized by prominent, well-defined arms. These arms appear to originate close to the central bulge and extend outwards. The spiral arms are moderately tightly wound, indicating a possible intermediate stage of spiral structure development. The galaxy's color profile suggests active star formation within the arms, evident in the presence of bluer, younger stellar populations. The central bulge shows a yellow hue, indicative of older stellar populations. The bulge is moderately sized, neither overwhelmingly dominant nor negligible in the galaxy's overall structure. There's no readily apparent bar structure traversing the galactic center. The disk is not viewed perfectly edge-on, allowing for clear observation of the spiral arms. Furthermore, the galaxy doesn't appear to be undergoing any major merging events or significant tidal disturbances. The galaxy is relatively smooth, without major irregularities.
