The galaxy presents a morphology consistent with an elliptical type, exhibiting a relatively smooth light distribution with a high degree of central concentration. The axial ratio suggests a moderately flattened shape, not perfectly spherical. The galaxy displays a color gradient, becoming slightly redder towards the center. No distinct spiral arms or disk structures are discernible. There is a faint, extended halo surrounding the central region, indicating the presence of an older stellar population. The overall color profile suggests a population of evolved stars with relatively low ongoing star formation.
