The galaxy presents as a somewhat elongated, smooth object with a central concentration of light. Its overall color appears reddish, indicative of a population of older stars. A bluer halo surrounds the central region, suggesting the presence of a younger, hotter stellar population. There are no obvious spiral arm structures or dust lanes visible at this resolution, suggesting it is likely an elliptical or lenticular galaxy. There appears to be little in the way of significant tidal disturbances or interactions with nearby galaxies. The morphology is generally undisturbed, with no major signs of mergers or significant disruptions.
