The galaxy presents as a smooth, elongated structure with a cigar-shaped morphology. Its light distribution appears relatively uniform, lacking prominent spiral arms or distinct features within its disk or bulge. Color gradients are subtle, shifting from a slightly bluer central region to a redder hue towards the outer edges. There is no obvious indication of an active galactic nucleus or intense starburst activity, although some low levels of star formation seem likely. Based on its overall appearance, the galaxy is likely a relatively evolved system that is not currently undergoing major mergers. Minor gravitational disturbance is possible, but any major disruption would be considered unlikely.
