The galaxy presents a generally smooth, elliptical morphology. It appears moderately compact with a bright, concentrated central bulge region exhibiting a yellowish hue, potentially indicating an older stellar population. The outer regions of the galaxy display a fainter, more diffuse distribution of light, possibly indicating a lower stellar density. The overall shape is more rounded than elongated, with no apparent signs of strong tidal disturbances or ongoing major merger activity. There may be some very subtle indication of a weak disk component.
