The galaxy presents as a centrally concentrated, largely featureless elliptical galaxy, exhibiting a smooth, round morphology. The galaxy's color profile suggests a stellar population dominated by older stars, with a yellowish-red hue indicative of lower star formation activity. There is minimal evidence of spiral arms or a pronounced disk structure. Faint blue regions may exist, but they are not well-defined. No significant tidal tails or obvious signs of recent major merger activity are apparent, though subtle disturbances cannot be ruled out.
