The galaxy presents a largely smooth, elliptical morphology. There is a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. This bulge fades gradually into an extended halo. The overall shape is mostly rounded, yet has some asymmetry suggestive of minor disturbances, possibly a small ongoing interaction or the aftermath of a past merger. Within the halo, there are subtle hints of clumpy structures, possibly regions of moderate star formation activity, which are further supported by the blueish colors detected in the outer regions. A substantial fraction of the galaxy appears undisturbed, indicating that while some interactions may have occurred, they have not drastically altered the overall structure. 
