The galaxy presents as an elongated, disk-shaped structure with a noticeable central bulge. The primary color of the bulge appears to be yellow, suggesting a concentration of older stellar populations. The disk exhibits a bluer hue than the central bulge, possibly indicating ongoing star formation, though this activity seems relatively subdued. The galaxy's structure appears smooth, lacking prominent spiral arms or significant dust lanes. There is no obvious evidence of tidal tails or strong gravitational disturbances, although a slight asymmetry is present. The overall morphology suggests a galaxy that is transitioning towards a more quiescent state with minimal recent star formation. The galaxy's apparent size is modest.
