This galaxy exhibits a somewhat irregular morphology, showing some features that indicate a disturbed structure. The light distribution appears relatively smooth, with a hint of a disk-like structure, although not sharply defined. There's evidence of ongoing or recent interaction or merging, with a portion of the galaxy appearing asymmetric. The bluer color suggests the presence of younger stellar populations and ongoing star formation activity. It is difficult to classify this galaxy as a standard elliptical or spiral based on the observed image due to the disturbed morphology, but the color would suggest it is not a standard eliptical galaxy. The shape of the galaxy deviates from being perfectly round, leaning towards a cigar-like shape.
