The galaxy presents as a relatively smooth and concentrated object, appearing largely elliptical in shape. A bright central bulge is visible, suggesting a high concentration of stars in the galactic nucleus. The galaxy exhibits a radial color gradient, with the central region appearing whiter and transitioning to a slightly redder hue in the outer regions. There is no apparent spiral arm structure or significant dust lane features visible in the image. Faint, diffuse light surrounds the central core, implying the presence of a stellar halo. The overall morphology indicates a mature system, potentially with a relatively low current star formation rate. No significant signs of ongoing mergers or tidal disturbances are immediately apparent, suggesting the system is relatively undisturbed.
