The galaxy appears as a relatively smooth, centrally concentrated object, consistent with an elliptical or lenticular morphology. The light distribution suggests a high degree of central concentration, fading gradually toward the edges. There is little evidence of spiral arms or distinct features such as prominent dust lanes. The overall color appears slightly redder, indicative of an older stellar population and/or a higher redshift. No significant signs of ongoing merger activity or strong tidal disturbances are apparent. The galaxy has a fairly round shape in projection, with only a slight hint of ellipticity.
