The galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated central bulge.  The light distribution appears centrally concentrated with an approximate apparent magnitude of around 15.5 in the r-band when accounting for redshift.  There is a gradual decline in intensity towards the outer regions, lacking any distinct spiral arm structures or prominent dust lanes. The galaxy shape has a slight flattening, as it is not perfectly circular. The overall color is somewhat redder, suggestive of an older stellar population. This redder color is more pronounced in the central regions with a slight gradient towards the outer edge. There is no visual evidence of significant ongoing star formation, implying that it is a relatively quiescent system. There are no signs of any recent major mergers or tidal disturbances.
