The galaxy presents as an elliptical morphology with a prominent central bulge. The light distribution is smooth, suggesting an older stellar population. The core exhibits a yellowish hue, indicating the presence of evolved stars. A slight asymmetry in the outer regions suggests a possible past or ongoing minor interaction or disturbance. There appears to be an area of redder light at the edge of the galaxy. The galaxy is neither perfectly round nor highly elongated, having a shape in between. There are no clear signs of strong tidal features, major mergers, or significant disk structures.
