The galaxy presents as a luminous object with a distinct, elongated shape, appearing more cigar-shaped than perfectly circular. The light distribution suggests a smooth profile, with a concentrated central bulge that gradually fades towards the outer edges.  There's a noticeable color gradient, shifting from bluer tones in the center to redder hues on the outskirts, potentially indicative of an older stellar population in the outer regions. This object is most likely an elliptical galaxy with an estimated stellar mass on the order of 10^10 solar masses and moderate levels of star formation. Slight asymmetry hints at possible past interactions or minor disturbances. 
