The galaxy presents as an elongated, spindle-shaped object, suggesting an elliptical morphology or a spiral galaxy viewed edge-on. Its light is concentrated toward the central region, indicating a prominent bulge. The color distribution appears to be relatively uniform, with a yellowish-orange hue dominating the core. This implies an older stellar population with a lower rate of ongoing star formation. There is some evidence of faint, diffuse material extending outwards from the main body, possibly representing a halo or tidal features. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or active galactic nuclei.
