The galaxy exhibits a generally elliptical morphology, appearing elongated with a high degree of central concentration. The central bulge is bright and appears to be composed of older stellar populations, indicated by its yellowish-white hue. A fainter, more diffuse disk component surrounds the bulge, showing a subtle transition in color. The color suggests the presence of a mix of stellar populations. The overall structure is relatively smooth, with minimal evidence of strong spiral arms or irregular features. There might be some faint tidal tails or disturbances. Indications of a possible minor merger or interaction with another smaller object are seen with a yellowish glow.
