The galaxy appears to be an elliptical type, exhibiting a smooth, diffuse light distribution without prominent spiral arms or a well-defined disk structure. The shape is moderately elongated, appearing more "in-between" than perfectly round or cigar-shaped. The central region presents a higher concentration of light, gradually fading towards the outer edges. There is no obvious presence of a strong, active galactic nucleus. The overall color is a pale blue, suggesting a population of relatively young, hot stars or ongoing star formation, though the smooth morphology and lack of distinct features typically indicate a more evolved system. There is some suggestion of a minor disturbance, but nothing that clearly indicates an active merger.
