The galaxy presents a largely smooth, elliptical appearance, with a concentrated central bulge. The light distribution suggests a fairly uniform stellar population. There is a minimal presence of spiral arm structures or significant dust lanes. The galaxy exhibits an overall round morphology, with a hint of elongation along one axis. No signs of ongoing major merging events are visible. Faint color gradients are present, with the core exhibiting a somewhat yellower hue, potentially indicating an older stellar population. Based on its red color, the galaxy appears to be a quite massive galaxy with minimal active star formation.
