The galaxy presents a somewhat irregular morphology. It appears to exhibit a degree of central concentration, although not definitively spherical. The overall structure appears to be complex, possibly indicative of a recent or ongoing interaction or merger event. A prominent feature is the presence of multiple regions of enhanced emission. The light distribution is not uniform; there is some clumpy substructure within the central regions and the outer regions, which may be indicative of active star formation or tidal features resulting from gravitational interaction. The colors appear to vary across the galaxy, ranging from bluer hues in some of the outer structures to redder or yellower tones toward the central region. The galaxy appears to have a significant mass and moderate to high star formation activity, with some evidence of recent merging.
