The galaxy presents as a slightly elongated, diffuse object. Its central region appears brighter and more concentrated, suggesting a prominent galactic nucleus. A subtle color gradient is observable; the central region exhibits a warmer, yellowish-white hue, potentially indicating an older stellar population or a higher concentration of dust. Moving outward from the core, the galaxy fades in intensity with a slight bluish tint, perhaps indicative of ongoing star formation in the outer regions. There appears to be a minor disturbance or potential interaction occurring, causing asymmetry in the morphology. While seemingly smooth, there are subtle irregularities in its shape.
