The galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, indicating a prominent bulge. The bulge region displays a yellowish hue, potentially indicative of an older stellar population. Fainter, bluer extensions emanate from the central bulge, hinting at the presence of a faint disk component. No distinct spiral arm structure or significant dust lanes are discernible in this image. The galaxy exhibits a relatively high degree of rotational symmetry and no apparent signs of major mergers or tidal disturbances. The galaxy appears to be a relatively isolated system.
