The galaxy presents a generally smooth morphology, appearing somewhat elliptical in shape. The central bulge is prominent and exhibits a yellowish-white hue, indicative of an older stellar population. Fainter, bluer regions are visible extending outwards from the center, possibly suggesting areas of more recent star formation within a disk component. The galaxy is not perfectly round, displaying a slight elongation. There may be some tidal disturbances visible, perhaps from a minor disturbance event. Based on the observed color gradient, this galaxy likely resides at an intermediate redshift. The galaxy is relatively isolated, with no other major galaxies appearing in immediate proximity that would suggest ongoing merger activity.
