The galaxy appears to be a single, relatively compact object with a somewhat elliptical shape. It presents a smooth, featureless morphology suggesting an older stellar population or a system that has undergone significant merging activity in the past. The light distribution is concentrated towards the center, exhibiting a radial falloff in intensity. Color gradients are present, showing a tendency toward redder hues at the core and a bluer periphery, possibly indicating on-going star formation in the outer regions. There are a few faint, diffuse extensions that may be indicative of tidal interactions. Overall, this galaxy appears to be an evolved system undergoing relatively low rates of star formation.
