The galaxy presents as a somewhat diffuse, moderately luminous object. Its overall morphology appears disrupted, possibly indicative of an ongoing or recent interaction. The central region shows a higher concentration of light with a yellowish-white hue, suggesting an older stellar population. Two distinct, more reddish concentrations of light are observed slightly offset from the main body, these may indicate regions of intense star formation or potentially tidally disrupted dwarf galaxies. There is a faint, extended halo around the galaxy with a slightly bluer color, which would indicate a population of younger stars. A notable degree of asymmetry is present in the galaxy's outer regions. Overall, the galaxy exhibits characteristics consistent with a system undergoing significant evolutionary changes, possibly influenced by gravitational interactions.
