The galaxy appears as a moderately luminous, relatively compact object. It exhibits a generally smooth morphology, with a predominantly elliptical shape. The light distribution is concentrated toward the center, with a gradual decrease in intensity outwards. There is a subtle yellow-orange color gradient, suggesting an older stellar population. No distinct spiral arms or features associated with active star formation are clearly visible. There appears to be little or no tidal disturbance or evidence of ongoing or recent major merger activity. The structure overall indicates a fairly well-settled, evolved system.
