The galaxy presents as a slightly inclined, disk-dominated system. It exhibits a smooth, elongated morphology, with a bright central bulge region that appears relatively symmetrical. The color gradient suggests a transition from bluer hues in the outer regions of the disk to redder colors toward the central bulge, potentially indicating differing stellar populations or dust content. There is subtle asymmetry to the outer disk's extent, possibly due to tidal interactions or internal processes influencing star formation. No prominent spiral arm structures or strong dust lanes are immediately apparent from the imagery alone. The galaxy's overall appearance is indicative of a morphology intermediate between a lenticular and a spiral type.
