The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. Its overall shape is elongated, appearing cigar-shaped rather than perfectly round. The light distribution indicates a concentration of older stellar populations, giving it a yellowish hue, particularly in the central region. There is a faint, diffuse disk structure. The galaxy does not appear to show any signs of significant ongoing mergers or major disturbances. There might be some minor irregularities or faint features that suggest possible interactions, but these are not clearly discernible.
