The galaxy appears to be a lenticular or early-type spiral, seen at an oblique angle relative to our line of sight. A central bulge is visible, exhibiting a yellowish-white hue, suggesting an older stellar population. The surrounding disk appears relatively smooth with hints of a spiral structure. Some regions within the disk show a bluer color, potentially indicating ongoing star formation. Faint tidal features or minor disturbances are possibly present, suggesting past or ongoing interactions with other galaxies. The overall shape of the galaxy is elongated, indicating a flattened structure. The galaxy lacks a significant amount of dust, as expected for its morphological type.
