The galaxy presents a relatively compact morphology. The central region exhibits a bright, somewhat amorphous structure. A faint, diffuse halo surrounds this core, extending outwards but lacking well-defined spiral arms. The color distribution is not uniform; the central region appears bluish-green suggesting recent or ongoing star formation, while more external regions trend toward redder hues. There is a possible interaction occurring, with a disturbance to the smoothness of the main galactic body and a possible second nucleus nearby, or perhaps simply an area of intense star formation. The outer halo appears irregular, suggesting a dynamically active system, potentially undergoing minor merger or tidal disruption.
