The galaxy presents a roughly elliptical morphology, with a brighter, more intensely luminous core region. The color distribution suggests active star formation, with blue hues dominating the central area, possibly indicating the presence of young, hot stars. There is a visible transition in color outwards from the center, shifting towards greenish-yellow tones. The galaxy doesn't exhibit a distinct spiral arm structure or a well-defined disk. Its outer edges are somewhat irregular, hinting at possible interactions or disturbances. Overall, the galaxy appears to be actively evolving, potentially undergoing recent or ongoing merger events with other galactic systems.
