The galaxy presents as an elliptical morphology, elongated with a cigar-shaped appearance. A smooth, diffuse light profile is observed, lacking prominent spiral arms or distinct features. The color distribution suggests a dominant population of older stars, exhibiting a yellowish-orange hue concentrated towards the galactic center, which is likely due to the accumulation of light from Population II stars. There is little indication of active star formation within the galaxy. The structure is largely undisturbed, with no obvious signs of major mergers or tidal interactions. Minor disturbances cannot be ruled out.
