The galaxy presents as a somewhat amorphous structure with a generally elliptical shape, spanning approximately 6 kiloparsecs in diameter. The light distribution within the galaxy appears relatively smooth, suggesting it may be an early-type galaxy. The color gradient shows a central concentration of yellowish light, possibly indicative of an older stellar population. There is a subtle blueish halo in the surrounding area, suggesting the presence of younger stars. The morphology indicates some level of gravitational disturbance, possibly a past or ongoing minor merger event. A possible merger is the most likely explanation for the two visible concentrations of light that appear to be interacting. The stellar mass is estimated to be substantial and it is currently experiencing a moderate rate of star formation.
