The galaxy appears as an elliptical or lenticular-type galaxy, exhibiting a smooth, centrally concentrated light profile. The galaxy shows a slightly elongated morphology, appearing cigar-shaped rather than perfectly circular. There is evidence of a possible minor disturbance in the galaxy's structure, possibly due to an ongoing or past interaction with another galaxy. The color gradient transitions from a yellowish-orange core to a redder outer halo, suggesting an older stellar population is more dominant in the central region. The galaxy's reddish color indicates the presence of relatively little active star formation.
