The galaxy appears to be an elliptical type, with a smooth, centrally concentrated light distribution. It exhibits a somewhat elongated shape, with the major axis extending roughly vertically in the image. The core region is bright and featureless, fading gradually towards the outer edges, with no apparent spiral arms or dust lanes visible. The overall color suggests a population of older stars, exhibiting a yellowish hue. There is no evidence of ongoing major mergers or significant tidal disturbances based on its morphology. Faint hints of a disk component may be present, but these features lack prominence.
