The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a centrally concentrated bulge with a smooth, diffuse halo. The color gradient transitions from a yellow-white core to a bluer outer region, which may indicate some ongoing, albeit moderate, star formation in the extended disk. There is no clear evidence of spiral arm structures. The galaxy exhibits a generally rounded, but slightly elongated shape, suggesting it could be an E4-E5 type elliptical or a nearly edge-on S0. There are no apparent signs of major mergers or significant tidal disturbances. The relatively smooth profile hints that the galaxy is likely relatively evolved with well mixed stellar populations. The intermediate redshift suggests this is a relatively distant galaxy.
