The galaxy presents a predominantly smooth morphology. It appears centrally concentrated with a yellowish hue, potentially indicating an older stellar population or a higher degree of dust obscuration. The overall shape appears largely elliptical, with a slight extension or cigar shape. There is a hint of faint, diffuse features extending outwards from the central region; potentially a disk or tidal features. There's no strong evidence of any active merging events, though some minor disturbances cannot be entirely ruled out. The galaxy exhibits a low rate of star formation, consistent with its redder color and smooth morphology. The estimated stellar mass of the galaxy is substantial.
