The galaxy presents a generally smooth morphology with a bright, concentrated central bulge. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears to be elliptical in shape, with a moderate degree of ellipticity. Color gradients suggest a relatively old stellar population, with a redder hue dominating the bulge and a subtle bluer tint in the outer regions. The galaxy shows a strong central concentration of light, fading gradually towards its edges. There is no clear indication of ongoing major mergers or tidal disturbances.
