The galaxy presents a predominantly smooth morphology. It appears as an elliptical or lenticular galaxy due to its overall shape. The primary color is a yellowish-white, indicative of an older stellar population and diminished ongoing star formation. There is little evidence of spiral arms or prominent dust lanes, supporting the classification of a galaxy with a smooth structure. The galaxy's core is only slightly brighter than the surrounding halo, implying a gradual increase in stellar density toward the galactic center. There appears to be no strong indication of recent or ongoing major mergers, though faint distortions suggest minor gravitational interactions.
