The galaxy appears as a lenticular or edge-on spiral type. It presents with a central bulge that is bright and appears relatively smooth, fading into a disk-like structure. The disk exhibits a blue-ish color profile suggestive of some ongoing star formation regions. This galaxy seems to be moderately inclined to our line of sight, offering a slightly oblong shape. Some asymmetry is visible, possibly indicating some tidal interactions or minor disturbances, but it is not a strong effect. It may also be due to the slight presence of dust lanes. The core may contain an older stellar population, while the disk shows characteristics of younger, star-forming regions. Based on the faintness of the disk it can be inferred that the star-forming region is minimal.
