The galaxy presents as an elliptical morphology, with a smooth and centralized light distribution. The object exhibits a distinct yellow-orange hue, suggesting a relatively older stellar population with lower rates of recent star formation. There is no obvious disc structure or spiral arms visible. The galaxy appears to have a high degree of central concentration, with brightness gradually decreasing from the core outwards. The outer edges are diffuse, blending smoothly into the background. The morphology is consistent with an elliptical galaxy undergoing little or no active merging or significant disturbances. The galaxy displays a slight elongation, appearing more "in-between" round and cigar shaped.
