The galaxy presents a primarily smooth and centrally concentrated morphology. The light distribution suggests a predominantly elliptical or lenticular classification. The central region exhibits a bright, yellowish-white core, indicative of an older stellar population or a possible active galactic nucleus. The outer regions show a gradual decrease in surface brightness, with a subtle, asymmetric extension towards the lower left. The overall color profile suggests a relatively passive star-forming environment. There is a minor hint of a disturbed morphology, potentially due to a past or ongoing minor interaction.
