The galaxy appears to be a relatively smooth, elliptical type, with a high degree of central concentration. Its morphology is largely spheroidal. The galaxy exhibits a dominant, yellowish core that transitions to a less intensely colored, more diffuse halo. There are no apparent spiral arms or obvious disk-like features. Based on the object's red color and lack of clear structure, the galaxy likely has a modest rate of ongoing star formation. There is no evidence of any major tidal disturbances or ongoing mergers, although there may be some minor irregularity on its edges, or minor disturbances within the galaxy. The galaxy presents a fairly uniform profile suggesting it is viewed face-on.
