The galaxy presents a relatively smooth morphology, with a possible faint disk structure. It appears slightly elongated, exhibiting an intermediate axis ratio. There is no indication of spiral arms. There are no obvious signs of major disturbances or ongoing mergers. A color gradient appears to be present, with the core region displaying a yellowish hue, possibly indicating an older stellar population. The outer regions show bluer tints which suggest younger stars exist in the surrounding area of the galaxy. Based on the faint disk structure, it is likely that this galaxy has a relatively small amount of current star formation, and may be tending towards a lenticular galaxy morphology.
