This galaxy presents a largely smooth, elliptical morphology. A dominant, centrally concentrated bulge is visible, exhibiting a yellowish-orange hue. This central region appears well-defined and relatively homogenous in color. A fainter, similarly colored, smaller region appears offset from the central bulge, possibly indicative of a minor interaction or remnant core. While the system is overall smooth, there may be some subtle disturbances in the outer regions. The overall shape is slightly elongated, but largely rounded. Any evidence of spiral arms or disk structures is absent. The system appears to be in the process of merging. The color suggests an older stellar population, with a possible lower rate of on-going star formation activity.
