The galaxy appears to be a relatively compact object, exhibiting a generally smooth morphology. There is a discernible central concentration of light, which may indicate a bulge component. The overall shape is somewhat elongated, suggesting a possible disk-like structure or a prolate spheroid. The color appears to be a slightly yellowish-white, potentially indicative of an older stellar population, though the presence of some bluer regions suggests ongoing or recent star formation. There are subtle irregularities in the light distribution, which could be faint spiral arms or tidal features, but they are not very pronounced. Based on its redshift, this is a relatively distant galaxy. There are no obvious signs of a major ongoing merger or significant tidal disruption, but the galaxy does have what appears to be another, small, spherical, yellow galaxy in its proximity, suggesting they may be gravitationally bound. 
