The galaxy presents as an elongated, cigar-shaped system, likely an elliptical galaxy viewed at an oblique angle or a spiral galaxy viewed edge-on. The central region exhibits a concentrated luminosity, suggesting a dense galactic nucleus or bulge. The galaxy's light appears relatively smooth, indicative of an older stellar population and reduced star formation activity. Faint bluer fringes are present along the edges, indicative of a small amount of recent star formation. There is no significant indication of major disturbances or active galactic nuclei activity based on the image.
