The galaxy presents a generally smooth and elliptical morphology. A slight elongation is visible, suggesting a classification leaning toward an S0 or elliptical galaxy. The color profile exhibits a yellow-red hue, indicating a stellar population that is predominantly older and redder, with minimal ongoing star formation. There appears to be no significant dust lane or spiral arm structure visible, reinforcing the classification as a relatively evolved system. A minor disturbance or faint tidal feature is not ruled out based on the fuzzy edges of the object. The light profile appears to have a high degree of central concentration.
