The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, surrounded by a fainter, more diffuse halo or disk. There is little discernible structure such as spiral arms or prominent dust lanes. The galaxy appears roughly rounded, with a slight deviation towards an in-between shape rather than perfectly circular or elongated. The galaxy exhibits a color gradient, transitioning from a yellow hue towards the central region to a more reddish color in the outer regions. This color suggests an older stellar population dominating the bulge, with potentially ongoing, albeit low, levels of star formation in the outer disk. No significant signs of mergers or tidal disturbances are apparent in the image.
