The galaxy presents as an elliptical morphology, with a smooth, largely featureless appearance. The light profile exhibits a centrally concentrated bulge region that is characterized by a yellowish-white hue, indicative of an older stellar population. Surrounding the bulge is a fainter, more diffuse halo of bluish light, which may indicate regions of more recent star formation activity, or a distinct population of stars. The galaxy displays a moderate redshift, suggesting it is at a significant cosmological distance. The overall shape tends to be in between round and cigar shaped, with a slight elliptical elongation. There appears to be no evidence of spiral arm structures or any significant disturbances from merging events.
