The galaxy presents as a lenticular or edge-on spiral with a smooth, elongated morphology. There is an apparent central bulge. The blue hue suggests the presence of some ongoing, albeit modest, star formation. This is likely concentrated within the disk, rather than throughout the entire structure. Faint dust lanes, while not sharply defined, may be present. There is no strong evidence of interaction with another galaxy, such as tidal tails or distorted morphology, and it appears relatively isolated within its environment. The axial ratio suggests a highly inclined disk, potentially near to edge-on, obscuring detailed features like spiral arms. The overall appearance indicates a galaxy transitioning, or already transitioned, to a more quiescent state, where star formation is suppressed.
