The galaxy presents as a relatively compact object with a diffuse, smooth morphology. The light distribution appears centrally concentrated, showing a brighter core region that gradually fades into the outer regions. There is minimal evidence of spiral arm structures or distinct features indicative of ongoing major star formation, and the overall color appears slightly redder than expected for a typical star forming galaxy. There is some minor possibility of a small interaction but there is no strong evidence. It likely has an elliptical shape.
