The galaxy appears to be undergoing a significant interaction, possibly a merger. Two distinct luminous components are observed, each exhibiting a relatively smooth morphology. One component presents a more concentrated central brightness, suggesting a well-defined core, while the other appears slightly more diffuse. A faint bridge of material seems to connect the two components, indicating gravitational interaction. The galaxy exhibits a relatively round shape, but displays some irregular features likely due to the ongoing interaction. Overall, the color appears to be dominated by yellow light, with only small hints of bluer light. This suggests a population of older stars with a low ongoing star formation rate.
