The galaxy presents a complex morphology, potentially indicative of an ongoing or recent interaction or merger event. The central region displays a relatively bright, compact core exhibiting a blue-shifted color profile. This suggests a concentration of younger, hotter stars or active galactic nucleus activity. Extending from the central region is a more diffuse structure, with a fainter luminosity gradient. The color in this outer region appears redder relative to the core, implying an older stellar population. There is an irregular morphology within the diffuse structure, characterized by asymmetries and possible tidal features, such as faint extensions or distortions. These features are suggestive of gravitational interactions, such as a possible minor merger event. The overall light distribution hints at disturbances to a potentially originally disk-like structure. The galaxy does not appear to have a high degree of rotational symmetry, suggesting that it may not be well relaxed dynamically.
