This galaxy appears to be an elliptical system, with a generally smooth and spheroidal morphology. The core of the galaxy exhibits a concentrated, bright luminosity. The light distribution suggests that the galaxy is dominated by an older stellar population, inferred from the yellowish-red hue. There is potential evidence of minor tidal disturbances or interactions visible as slight distortions in the galaxy's outer regions, possibly indicating past or ongoing merger events. The object is moderately round in shape. The system does not appear to be actively forming many stars.
