The galaxy appears to be a relatively smooth, centrally concentrated system with a slightly elliptical morphology. The light profile transitions smoothly from a bright, compact core to a fainter, more diffuse halo. The color gradients suggest a redder core, with bluer hues becoming more prominent in the outer regions. There is no evidence of a prominent disk component or spiral arm structure. Faint tidal features or minor disturbances are potentially present, which could indicate a past or ongoing interaction. The overall color of the galaxy is moderately red. The apparent size is small; at a distance implied by its redshift, it is likely to be an intermediately sized galaxy in terms of physical extent.
