The galaxy presents as a single, relatively smooth object. There appears to be little to no discernible spiral structure, barring the faint, disk-like structure. The light from the galaxy appears to be largely homogeneous with a small amount of color variation. The object is centrally concentrated, displaying no significant asymmetries or tidal features indicative of recent major merger activity, though minor disturbances may not be visible at this resolution. The shape of the galaxy is mostly round in appearance. There is no pronounced bar feature or ring structure detected. Color gradients suggest it is likely an evolved system with ongoing star formation. The galaxy exhibits a reddish hue which, along with the redshift measurement, is consistent with an aging stellar population and a significant distance.
