The galaxy presents as an elongated, elliptical structure. The light distribution appears smooth, with a concentrated central bulge exhibiting a yellowish-white hue. Moving outward from the core, the light gradually decreases in intensity, transitioning towards a reddish-orange tone at the edges. The galaxy does not show any prominent spiral arm structures, nor are there any obvious signs of significant dust lanes or regions of active star formation visible. The overall morphology suggests an evolved stellar population and a system largely devoid of ongoing major mergers.
