The galaxy appears to be a lenticular or early-type spiral galaxy at an estimated distance corresponding to a redshift of approximately 0.16. The central bulge region exhibits a smooth, concentrated luminosity profile, appearing yellowish-white in color, suggesting a population of older stars. The outer regions of the galaxy show a more diffuse, bluish hue, potentially indicating the presence of some ongoing or recent star formation, although the overall morphology is dominated by the spheroidal bulge component. There are no distinct spiral arms or bar structures visible. The galaxy's shape is approximately elliptical, with a slight deviation from perfect circularity. There are no obvious signs of tidal interactions or mergers, although subtle asymmetries could be present upon closer inspection with higher resolution imaging.
