The galaxy appears as a centrally concentrated object with a generally smooth morphology. The light profile suggests an elliptical or lenticular galaxy. The core is bright and appears yellowish/reddish, surrounded by a faint, diffuse halo. The apparent roundness of the galaxy indicates it is likely not a spiral seen edge-on. There is minimal evidence of spiral arm structure or significant dust lanes. There are no apparent signs of a major ongoing merger, although subtle disturbances within the halo cannot be ruled out definitively. The color suggests a stellar population dominated by older, redder stars. There are hints of some green light possibly indicating some star formation, but overall, the galaxy does not seem to be undergoing intense star formation.
