The galaxy presents as a relatively smooth, elongated structure. The color profile suggests a bias towards older stellar populations, with a predominantly blueish-white hue across the main body, indicating the presence of some younger, bluer stars within the galaxy, while the light is generally redder than the blue. There is no spiral structure, obvious dust lanes, or knots of star formation visible. The galaxy appears relatively undisturbed, with no strong evidence of major mergers or tidal interactions. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the edges. The galaxy appears to be a flattened spheroid, seen nearly edge-on, but the smoothness suggests this object is either an elliptical galaxy or perhaps a lenticular galaxy.
