The galaxy presents a generally smooth, elliptical morphology. It appears relatively round in shape, with no discernible spiral arm structure or a prominent disk. The light distribution is centrally concentrated, exhibiting a gradual decrease in intensity from the core outwards. There are no obvious signs of recent major merger activity or significant tidal disturbances. There may be a faint dust lane visible within the galaxy. The overall color of the galaxy appears to be reddish, suggesting an older stellar population and a lack of significant ongoing star formation.
