This galaxy presents as a lenticular, disk-shaped system, observed at an oblique angle relative to our line of sight. The central region exhibits a smooth, concentrated luminosity profile, likely indicative of a bulge. The disk appears relatively thin and extended. There is a slight hint of spiral structure. The galaxy displays a color gradient, transitioning from bluer hues in the disk to redder tones in the central bulge. The bluer colors suggest ongoing star formation. The galaxy does not show signs of major tidal disturbances or active galactic nuclei, nor does it appear to be undergoing a major merger event. The galaxy's morphology suggests that it could be evolving from a spiral galaxy to an elliptical galaxy.
