The galaxy presents a roughly elliptical morphology, appearing elongated along a vertical axis. The central region exhibits a bright, concentrated core, suggestive of a significant stellar population. Extending outward from the core, a more diffuse disk or halo-like structure is observed, displaying a gradient in surface brightness, with intensity decreasing away from the center. There are some subtle asymmetries and possible disturbances in the outer regions, hinting at possible interactions or internal dynamics. Colors are subdued but with an average light-bluish color. There is a faint elongated trail of light extending from the galaxy, but it's hard to determine whether the light comes from dust or stars. The overall appearance suggests a system that could be classified as an early-type spiral or possibly an elliptical galaxy with a slight disk component.
