The galaxy presents as a lenticular or perhaps even a spiral galaxy seen at a steep angle. The dominant feature is a smooth, elongated bulge exhibiting a gradient in luminosity. This indicates a relatively old stellar population with minimal ongoing star formation. A faint, flattened disk is visible extending from the bulge. The disk material appears somewhat disturbed, possibly due to gravitational interactions or internal processes. Patchy regions of redder color are apparent within the disk, which could indicate the presence of dust lanes or regions of recent, albeit limited, star formation. The overall appearance suggests a galaxy in a transitional phase, perhaps evolving from a spiral to a more quiescent elliptical-like morphology. Further spectroscopic data would be valuable to ascertain the precise redshift and chemical composition of this object.
