The galaxy presents as a centrally concentrated object with a relatively smooth, diffuse morphology. The light profile appears roughly elliptical, though its circularity is significant. The galaxy exhibits a color gradient, appearing bluer towards the central region. There is no clear evidence of spiral arm structure or a distinct galactic disk. Faint wisps or tidal features might be present, suggesting potential interactions or minor disturbances, although the image resolution limits certainty. The galaxy's overall appearance suggests a system undergoing active star formation, particularly within its core. It's likely a moderately massive system with a noticeable rate of on going star formation. There is a possibility of a minor merger event, but it is unclear from the picture.
