The galaxy presents a largely smooth, elliptical morphology. It appears highly rounded, exhibiting a uniform, concentrated light profile with no visible spiral arms or bar structures. The core region is bright and appears yellowish-white, suggesting a population of older stars. There is a color gradient, transitioning to a redder hue on one side, possibly indicating dust or a slightly younger stellar population in that region. No significant tidal features or signs of recent major mergers are apparent, although there might be subtle disturbances.
