The galaxy appears to be a lenticular or early-type spiral galaxy, likely at a redshift that places it at a considerable cosmological distance. The galaxy exhibits a smooth, centrally concentrated morphology. There is little to no apparent spiral arm structure or prominent dust lanes visible in the image, although very faint diffuse features may be present. The galaxy displays a centrally brightened bulge region, surrounded by a more diffuse and extended disk component. Color gradients suggest a predominantly older stellar population. The lack of strong blue emission implies a relatively low rate of ongoing star formation. The elongated shape indicates a non-spherical morphology, with an axial ratio that suggests it is viewed at an intermediate inclination. The smooth profile and lack of tidal features indicate that the galaxy is relatively undisturbed and is not undergoing a major merger event, although there may be minor asymmetry or subtle distortions present.
