This galaxy exhibits a primarily smooth morphology, with a notable fraction of its light concentrated in a central region. The object appears to have a generally round shape, though some subtle deviations from perfect circularity are present. Evidence suggests the presence of some internal structure, although it is not strongly defined, possibly indicating minor disturbances within the galaxy. The color profile reveals a range of stellar populations, with bluer light concentrated in the core region, and some slightly redder tones distributed more peripherally. There appears to be an indication of recent star formation. The overall impression is of a galaxy that is relatively massive and has features of possibly an ongoing, minor merging event. 
