The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The light distribution appears to be centrally dominant with a gradual falloff in intensity toward the outer regions.  There is a slight elongation but the shape is mostly round. There is no discernable disk-like structure or spiral arms. The galaxy exhibits a yellowish color, suggesting an older stellar population and relatively low current star formation activity. There is no evidence of any significant ongoing merger activity or major morphological disturbances. Overall, this galaxy appears to be a fairly quiescent, evolved system.
