The galaxy appears as an elliptical-like structure, exhibiting a relatively smooth morphology without prominent spiral arms or distinct features typically associated with disk galaxies. The light distribution suggests a high degree of central concentration. The galaxy's color profile appears to be dominated by redder wavelengths, indicative of an older stellar population with suppressed recent star formation. There is a slight elongation, but the galaxy is mostly round. There appears to be no prominent signs of ongoing mergers or major tidal disturbances. Overall, the morphology points toward a evolved system.
