The galaxy presents as a flattened spheroid in the image, appearing relatively small in angular size. The central region exhibits a bright, concentrated core, possibly indicating the presence of an active galactic nucleus or a dense stellar population.

A diffuse, extended halo surrounds the core, displaying a gradient in color. The inner regions of the halo appear bluish, suggesting younger, hotter stars, while the outer regions are more reddish, potentially due to older stellar populations or dust obscuration.

Evidence suggests a possible interaction or merger event. There are some features that could indicate minor tidal disturbances. Overall, the galaxy's morphology is not that of a pure elliptical or spiral, but instead a combination of traits, possibly indicating an ongoing or recent merger. A small fraction of light indicates the presence of a feature. 
