This galaxy presents a relatively compact morphology. It exhibits a bright, concentrated central bulge region that appears nearly spherical in projection. Surrounding the bulge, a fainter, more diffuse disk component can be observed, oriented approximately edge-on to our line of sight. There appears to be some dust obscuration along the plane of the disk, giving it a slightly irregular appearance.  A faint tidal tail seems to extend outwards from the primary body of the galaxy. There are also some signs that the galaxy may be interacting with something outside of the galaxy based on some of the visible irregularities. Further analysis of the color gradients within the disk and tidal tail, along with spectroscopic data, would be beneficial for understanding the galaxy's stellar populations and possible interaction history.
