The galaxy presents as a flattened, disk-like structure, oriented at an angle relative to our line of sight. The central region appears brighter and more concentrated, suggesting a bulge. The disk exhibits a smooth, somewhat diffuse appearance, with a notable lack of prominent spiral arm structure. A faint blue hue is observed throughout the galaxy, which indicates the presence of some young, hot stars. There are subtle asymmetries and disturbances in the outer disk region that are more prominent at one end of the object, indicating some sort of gravitational interaction with another object. Dust lanes are not clearly discernible, but the disk morphology suggests a relatively low dust content. Overall, the galaxy appears to be an intermediate spiral or lenticular type.
