The galaxy presents a predominantly smooth morphology, appearing elliptical in shape. The light distribution suggests a centrally concentrated profile, with a gradual decrease in intensity towards the outer regions. The galaxy exhibits a yellowish-orange hue, potentially indicative of an older stellar population and reduced ongoing star formation. There is no clear evidence of spiral arms or a well-defined disk structure. Minor asymmetry is present, but no major disturbances or merging features are apparent. The galaxy's estimated size is moderate, and the overall visual impression suggests a relatively evolved system.
