The galaxy presents an elliptical morphology, appearing largely smooth in structure without prominent spiral arms or a defined disk. It exhibits a central bulge with a slightly elongated shape. The color profile suggests a population of older stars, with a dominant yellowish hue. There is a hint of blue light that may represent the presence of some star formation. The estimated size of the galaxy is a few kiloparsecs in radius. There is no obvious evidence of a major ongoing merger, but there are some disturbances in the shape. The galaxy is moderately massive. There is weak star formation, relative to other galaxies. 
