The galaxy appears to be an elliptical, spheroidal system, exhibiting a relatively smooth and featureless structure. The light distribution suggests a concentration of older stellar populations, displaying a more reddish color profile, primarily in the central regions. The overall shape is predominantly round with only minor deviations from perfect circularity. There is no evidence of prominent spiral arms, bars, or other disk-like features. There may be evidence of very minor disturbance in this galaxy system. It is likely a massive system with moderate levels of star formation activity.
