The galaxy presents a concentrated and moderately bright core, indicative of a substantial central mass concentration, possibly a supermassive black hole. The light profile suggests a smooth and somewhat elliptical morphology, with a dominant bulge component. The galaxy's color indices appear to be relatively red, suggesting an older stellar population or significant dust obscuration, potentially muting star formation within the galaxy. It displays minimal features of a spiral structure, if any. The galaxy is characterized by a relatively uniform distribution of light. There may be signs of tidal disturbances but these are difficult to confirm from this image alone. Overall, this galaxy appears to be a relatively evolved system nearing the end of its active star formation.
