This galaxy appears to be a disk galaxy, observed at a significant inclination, but not quite edge-on. A bulge is visible in the center, with a yellowish-white hue indicating an older stellar population. The disk surrounding the bulge exhibits a more mottled texture, likely due to a mixture of stellar populations and dust. Faint hints of spiral arm structure can be discerned, characterized by bluer tones, suggesting the presence of younger, hotter stars. There is no obvious major merger activity, and the galaxy appears relatively undisturbed with no strong tidal tails or bridges. The color distribution suggests a moderate level of star formation within the disk, though it seems to be less active than a typical spiral. There is little evidence of a pronounced dust lane. The galaxy appears to be relatively smooth, but also has some distinct features. The lack of a strong dust lane and the color of the bulge may mean it is close to an intermediate type galaxy, somewhere between a spiral and a lenticular galaxy.
