The galaxy appears to be a disk galaxy, potentially of an intermediate spiral type. There is a definite central bulge exhibiting a yellow color. The arms are faint and difficult to discern, but there are hints of spiral structure. Color gradients suggest older stellar populations are dominant, with a relatively small amount of ongoing star formation. A redder hue dominates throughout the disk with hints of blue light. The overall morphology suggests a mature galaxy, possibly with a substantial mass. The shape suggests the galaxy disk is tilted at a steep angle with respect to our line of sight. There is no obvious sign of a major merger event in the past. The galaxy appears relatively isolated and has a smooth appearance.
