The galaxy presents as an elongated structure, exhibiting characteristics consistent with a lenticular or possibly an edge-on spiral galaxy. There is a smooth, diffuse light distribution across the galaxy, with a subtle central concentration. Color gradients indicate a generally older stellar population across the galaxy. There may be a neighboring object nearby, which appears more yellowish in color, with a generally round shape. Based on its proximity and color, it is possible that this may be an interacting dwarf galaxy. There are no apparent tidal features to suggest any merger events. Based on the overall characteristics, this is likely a mature galaxy with suppressed star formation.
