The galaxy presents as a somewhat elongated elliptical structure, with a significantly brighter central region suggesting a concentration of older stars and possibly a supermassive black hole at the core. The primary color is a reddish-orange hue, indicative of an older stellar population dominated by red giants. The smooth appearance suggests a lack of significant recent star formation. A subtle blue tinge on the periphery suggests a small population of younger, hotter stars are present, perhaps in the outer regions. The morphology does not indicate any major disturbances or ongoing mergers.
