The galaxy appears as a centrally concentrated, elliptical or lenticular system. Its overall light distribution is smooth, lacking prominent spiral arms or irregular features. The core region exhibits a higher surface brightness, gradually decreasing outwards. The shape is largely consistent with being an elliptical galaxy, somewhere in between being perfectly round or a more elongated cigar shape. There is little evidence of ongoing mergers or major disturbances, with a significant amount of citizen scientists reporting the galaxy as undisturbed. The color indices suggest a relatively evolved stellar population, with a moderate amount of star formation.
