The galaxy presents as a relatively smooth structure with a bright, concentrated central bulge. A faint disk component is observed, though the spiral arm structure is not well-defined. The disk exhibits a bluer color than the central bulge, suggesting the presence of younger stellar populations. The galaxy appears to have a slight asymmetry, possibly indicating a minor interaction or disturbance. Overall, the galaxy is a mid-sized system, and it appears to have intermediate mass and star formation properties.
