The galaxy presents as a spiral type, with tightly wound spiral arms originating from a moderate-sized central bulge. The galaxy exhibits a relatively high degree of symmetry, with the spiral arms displaying a consistent morphology on both sides of the bulge. The disk appears inclined, suggesting a significant viewing angle relative to the galaxy's plane. The central bulge displays a brighter and more uniform luminosity profile than the surrounding disk. Faint star-forming regions are visible within the spiral arms, appearing as areas of slightly enhanced blue coloration. The galaxy shows no obvious signs of recent major merger activity, though some minor disturbances are apparent, possibly indicating a past interaction or accretion event. Overall, the galaxy appears to be a relatively undisturbed spiral, with ongoing star formation concentrated in its spiral arms. The color index suggests a relatively evolved stellar population overall, consistent with a classification as an intermediate spiral type.
