The galaxy presents as a relatively compact object with a somewhat diffuse morphology. The central region exhibits a pronounced concentration of light, appearing smooth and yellowish-orange in color, suggesting an older stellar population. Surrounding this core is a fainter, less defined halo or disk component. There are subtle color variations within the outer regions, but no distinct spiral arm structures are discernible. Some slight disturbances or asymmetries are observed, which could indicate minor gravitational interactions or internal dynamic processes. The galaxy's overall structure suggests an elliptical morphology, though some disk features may be present.
