The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution appears centrally concentrated, fading gradually towards the outer regions.  The core exhibits a reddish hue, suggesting a population of older, redder stars.  The outer regions show some evidence of bluer colors, potentially indicating areas of more recent star formation, although this is subtle.  The overall shape is somewhere between round and elongated. There is no strong evidence of significant tidal disturbances or ongoing merger activity. The galaxy is likely a fairly massive system, exhibiting low levels of ongoing star formation. 
