The galaxy appears as a centrally concentrated object with a largely smooth morphology. It exhibits a somewhat elliptical shape, appearing mostly round. The core region displays a yellowish hue, potentially indicative of an older stellar population.  There are very faint irregularities present with some subtle and minor disturbances visible. There is no strong evidence of recent or ongoing major mergers.  The galaxy shows no distinct spiral arm structure. It appears to be a relatively massive galaxy and quiescent with relatively little recent star formation.
