The galaxy presents a relatively smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that gradually fades into a diffuse halo. The isophotes appear elongated, suggesting a moderate ellipticity. No distinct spiral arm structures or prominent dust lanes are discernible. The color profile shows a subtle bluing towards the center of the galaxy, transitioning to redder hues in the outer regions. There may be evidence of minor gravitational disturbance.
