The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall color is bluish-white, suggestive of a population of younger, hotter stars, particularly in the central region. The galaxy's shape is somewhat elliptical, displaying a slight deviation from perfect circularity, but there is little evidence of a prominent disk structure or spiral arms. There's a subtle elongation, which is indicative of an elliptical morphology that is closer to in-between. The smooth morphology suggest a well-established galaxy. The color and morphology indicates ongoing or recent star formation activity. There is no sign of significant tidal disturbances or interactions that could be indicative of any major or minor mergers.
