The galaxy appears as a relatively compact, unresolved object. Its morphology suggests it is largely smooth, without prominent spiral arms or a distinct disk structure. It is mildly elliptical in shape, appearing somewhere between round and elongated. There is no obvious evidence of tidal disturbances or a major ongoing merger event. The color profile indicates it is more luminous in redder wavelengths, and less luminous in bluer wavelengths. This color suggests an older stellar population. Based on these observed properties, it is likely an elliptical galaxy. The estimated size based on its half light radius suggests that it is relatively small for an elliptical galaxy. Given the lack of significant blue light, the current star formation rate is low.
