The galaxy presents as a somewhat smooth, although slightly disturbed, system. It exhibits an irregular morphology, deviating significantly from a pure elliptical or spiral form. There are indications of possible tidal features or interactions, suggesting an ongoing or recent merger event, however the merger seems to be mostly resolved. The galaxy's color profile is dominated by redder hues with a slight yellow tint, possibly indicating an older stellar population and suppressed star formation activity. The overall light distribution appears concentrated, but with some extended, diffuse components.
