The galaxy appears to be composed of two distinct components: a larger, more diffuse, and centrally concentrated region, and a smaller, more elongated region positioned somewhat inferior to the main body. The primary component exhibits a smooth, featureless morphology, with a color profile suggesting an older stellar population. The inferior, elongated component displays a slightly bluer color, which could indicate younger stars or ongoing star formation. The overall appearance suggests a possible interaction or merger event, with the secondary component potentially a smaller galaxy being accreted by the larger one. There is little evidence of spiral arms or a well-defined disk structure. Based on its color and apparent lack of features, the dominant component may be an elliptical or lenticular galaxy.
