The galaxy presents as a generally smooth and rounded object with a concentration of light in the central region. The color gradient suggests a composition of older stellar populations, with a yellowish-red hue prominent in the core and surrounding regions. There appears to be evidence of a potential interaction or merging event. The shape appears disturbed, with at least two distinct bright clumps within the galaxy's body. Overall, it exhibits properties of a mature, massive system with ongoing or recent interaction activity.
