The galaxy presents as an elliptical morphology, demonstrating a smooth and centralized distribution of light. The core region exhibits a higher concentration of luminous material, appearing more intensely illuminated than the surrounding areas. The color profile indicates a general yellowish hue, potentially indicative of an older stellar population. There appears to be a lack of significant disk-like features or spiral arms, further supporting the elliptical classification. Slight irregularities are visible, perhaps showing minor disturbances. The overall structure is relatively undisturbed, with no major signs of ongoing mergers. The shape is rather round, not strongly elongated. The galaxy is relatively faint.
