The galaxy appears to be undergoing a significant interaction, possibly a merger, with at least one other galactic component. A main body of the galaxy displays a yellowish hue, suggestive of an older stellar population. This body presents a somewhat elongated, cigar-like shape, not fully spherical, indicating a departure from a relaxed elliptical morphology. A second distinct component, also yellowish, is observed in close proximity, suggesting it could be the core of another interacting galaxy. There is visible disruption to the overall structure, with signs of tidal tails or distorted arms emanating from the system, indicating gravitational disturbance. The bluer colors are observed within the regions of the merger and in the outer edges of the galaxy. Given the observed properties, this system likely experiences ongoing or recent star formation activity, especially within the merging region. The system exhibits a notable amount of internal structure, deviating from a smooth, featureless appearance, further supporting the classification as an interacting or merging system.
