The galaxy appears as a centrally concentrated, relatively smooth object with a moderate redshift. It exhibits a spheroidal morphology, showing a mostly round shape with a faint, diffuse halo. There is no obvious spiral arm structure or central bar visible. The light is dominated by redder wavelengths, suggesting an older stellar population and lower star formation rate. While generally smooth, there is subtle color variation across its extent. There are no apparent signs of ongoing or recent merger activity, nor any significant tidal disturbances.
