The galaxy appears as a somewhat irregular, centrally concentrated object. Its color profile suggests a generally older stellar population, dominated by redder hues, with potentially some regions of ongoing or recent star formation evidenced by slightly bluer tinges. The overall morphology is diffuse, suggesting a galaxy in the process of merging with another structure, or possibly a post-merger remnant. There is a hint of asymmetry in the distribution of light, which could be indicative of tidal interactions or disturbances. Overall, the galaxy exhibits characteristics suggesting a complex evolutionary history and a relatively high mass, with some current star formation, although subdued relative to its mass.
